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Artigo de periodico
The role of disk tearing and precession in the observed variability of pleione (2022)
Marr, K. C ; Jones, C. E. ; Tycner, C ; Carciofi, Alex Cavaliéri ; Silva, Fonseca A. C
Source: Astrophysical Journal. Unidade: IAG
Assunto: ESTRELAS BINÁRIAS
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MARR, K. C et al. The role of disk tearing and precession in the observed variability of pleione. Astrophysical Journal, v. 928, p. 145, 2022Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ac4266. Acesso em: 10 nov. 2024.
APA
Marr, K. C., Jones, C. E., Tycner, C., Carciofi, A. C., & Silva, F. A. C. (2022). The role of disk tearing and precession in the observed variability of pleione. Astrophysical Journal, 928, 145. doi:10.3847/1538-4357/ac4266
NLM
Marr KC, Jones CE, Tycner C, Carciofi AC, Silva FAC. The role of disk tearing and precession in the observed variability of pleione [Internet]. Astrophysical Journal. 2022 ;928 145.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
Vancouver
Marr KC, Jones CE, Tycner C, Carciofi AC, Silva FAC. The role of disk tearing and precession in the observed variability of pleione [Internet]. Astrophysical Journal. 2022 ;928 145.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
Artigo de periodico
Interferometric detections of sdO companions orbiting three classical Be stars (2022)
Klement, Robert ; Schaefer, Gail H; Carciofi, Alex Cavaliéri
Source: Astrophysical Journal. Unidade: IAG
Assunto: ESTRELAS BINÁRIAS
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KLEMENT, Robert e SCHAEFER, Gail H e CARCIOFI, Alex Cavaliéri. Interferometric detections of sdO companions orbiting three classical Be stars. Astrophysical Journal, v. 926, p. 213, 2022Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ac4266. Acesso em: 10 nov. 2024.
APA
Klement, R., Schaefer, G. H., & Carciofi, A. C. (2022). Interferometric detections of sdO companions orbiting three classical Be stars. Astrophysical Journal, 926, 213. doi:10.3847/1538-4357/ac4266
NLM
Klement R, Schaefer GH, Carciofi AC. Interferometric detections of sdO companions orbiting three classical Be stars [Internet]. Astrophysical Journal. 2022 ;926 213.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
Vancouver
Klement R, Schaefer GH, Carciofi AC. Interferometric detections of sdO companions orbiting three classical Be stars [Internet]. Astrophysical Journal. 2022 ;926 213.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
Artigo de periodico
NICER x-ray observations of Eta Carinae during Its most recent periastron passage (2022)
Espinoza-Galeas, David ; Corcoran, Michael ; Damineli Neto, Augusto
Source: Astrophysical Journal. Unidades: IAG, IF
Subjects: ASTROFÍSICA, EVOLUÇÃO ESTELAR
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ESPINOZA-GALEAS, David e CORCORAN, Michael e DAMINELI NETO, Augusto. NICER x-ray observations of Eta Carinae during Its most recent periastron passage. Astrophysical Journal, v. 933, p. 136, 2022Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ac69ce. Acesso em: 10 nov. 2024.
APA
Espinoza-Galeas, D., Corcoran, M., & Damineli Neto, A. (2022). NICER x-ray observations of Eta Carinae during Its most recent periastron passage. Astrophysical Journal, 933, 136. doi:10.3847/1538-4357/ac69ce
NLM
Espinoza-Galeas D, Corcoran M, Damineli Neto A. NICER x-ray observations of Eta Carinae during Its most recent periastron passage [Internet]. Astrophysical Journal. 2022 ; 933 136.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac69ce
Vancouver
Espinoza-Galeas D, Corcoran M, Damineli Neto A. NICER x-ray observations of Eta Carinae during Its most recent periastron passage [Internet]. Astrophysical Journal. 2022 ; 933 136.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ac69ce
Artigo de periodico
Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets (2021)
Medina-Torrejon, Tania ; Dal Pino, Elisabete de Gouveia ; Kadowaki, Luis H. S. ; Kowal, Grzegorz ; Singh, Chandra B. ; Mizuno, Yosuke
Source: Astrophysical Journal. Unidades: IAG, EACH, IF
Subjects: ASTROFÍSICA, MAGNETOHIDRODINÂMICA, RAIOS CÓSMICOS, ACELERAÇÃO DE PARTÍCULAS, NEUTRINOS
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MEDINA-TORREJON, Tania et al. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, v. 908, n. 2, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abd6c2. Acesso em: 10 nov. 2024.
APA
Medina-Torrejon, T., Dal Pino, E. de G., Kadowaki, L. H. S., Kowal, G., Singh, C. B., & Mizuno, Y. (2021). Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, 908( 2). doi:10.3847/1538-4357/abd6c2
NLM
Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
Vancouver
Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
Artigo de periodico
Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets (2021)
Kadowaki, Luis H. S. ; Dal Pino, Elisabete de Gouveia ; Torrejón, Tania Medina ; Mizuno, Yosuke ; Kushwaha, Pankaj
Source: Astrophysical Journal. Unidades: IAG, IF
Subjects: ASTROFÍSICA, RELATIVIDADE (FÍSICA), MAGNETOHIDRODINÂMICA, ACELERAÇÃO DE PARTÍCULAS, JATOS (ASTRONOMIA)
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KADOWAKI, Luis H. S. et al. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets. Astrophysical Journal, v. 912, n. 2, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abee7a. Acesso em: 10 nov. 2024.
APA
Kadowaki, L. H. S., Dal Pino, E. de G., Torrejón, T. M., Mizuno, Y., & Kushwaha, P. (2021). Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets. Astrophysical Journal, 912( 2). doi:10.3847/1538-4357/abee7a
NLM
Kadowaki LHS, Dal Pino E de G, Torrejón TM, Mizuno Y, Kushwaha P. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets [Internet]. Astrophysical Journal. 2021 ; 912( 2):[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abee7a
Vancouver
Kadowaki LHS, Dal Pino E de G, Torrejón TM, Mizuno Y, Kushwaha P. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets [Internet]. Astrophysical Journal. 2021 ; 912( 2):[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abee7a
Artigo de periodico
How Magnetic Activity Alters What We Learn from Stellar Spectra (2020)
Spina, Lorenzo ; Moreno, Jorge Luis Meléndez ; Galarza, Jhon J. Yana
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 10 nov. 2024.
APA
Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2020). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7
NLM
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Vancouver
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Artigo de periodico
Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 (2020)
Nascimento J.-D. do ; Almeida, L. de ; Velloso, E. N ; Anthony, F.; Costa, J. S. da; Castro, M; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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NASCIMENTO J.-D. DO, et al. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, v. 898, p. 173 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab9c16. Acesso em: 10 nov. 2024.
APA
Nascimento J.-D. do,, Almeida, L. de, Velloso, E. N., Anthony, F., Costa, J. S. da, Castro, M., & Moreno, J. L. M. (2020). Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, 898, 173 2020. doi:10.3847/1538-4357/ab9c16
NLM
Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
Vancouver
Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
Artigo de periodico
The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars (2020)
Cain,Madelyn ; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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CAIN, Madelyn e MORENO, Jorge Luis Meléndez. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, v. 864, p. 43 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 10 nov. 2024.
APA
Cain, M., & Moreno, J. L. M. (2020). The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, 864, 43 2020. doi:10.3847/1538-4357/aad37d
NLM
Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Vancouver
Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g (2020)
Garcia, A. ; Horvath, Jorge Ernesto
Source: Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS
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GARCIA, A. e HORVATH, Jorge Ernesto. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g. Astrophysical Journal, v. 903p. 75 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abb823. Acesso em: 10 nov. 2024.
APA
Garcia, A., & Horvath, J. E. (2020). A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g. Astrophysical Journal, 903p. 75 2020. doi:10.3847/1538-4357/abb823
NLM
Garcia A, Horvath JE. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g [Internet]. Astrophysical Journal. 2020 ; 903p. 75 2020[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abb823
Vancouver
Garcia A, Horvath JE. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g [Internet]. Astrophysical Journal. 2020 ; 903p. 75 2020[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/abb823
Artigo de periodico
The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 (2020)
Suffak,M W; Richardson, Noel D; Jones, C E; Tycner, C; Henry, G W; Carciofi, A C; Mota, B C; Rubio, A C
Source: Astrophysical Journal. Unidade: IAG
Subjects: TRANSFERÊNCIA RADIATIVA, ESTRELAS BINÁRIAS
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SUFFAK, M W et al. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, v. 890, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab68dc. Acesso em: 10 nov. 2024.
APA
Suffak, M. W., Richardson, N. D., Jones, C. E., Tycner, C., Henry, G. W., Carciofi, A. C., et al. (2020). The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, 890. doi:10.3847/1538-4357/ab68dc
NLM
Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab68dc
Vancouver
Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/ab68dc
Artigo de periodico
The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* (2020)
Ezzeddine, Rana; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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EZZEDDINE, Rana e MORENO, Jorge Luis Meléndez. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, v. 898, p. 150 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d1a. Acesso em: 10 nov. 2024.
APA
Ezzeddine, R., & Moreno, J. L. M. (2020). The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, 898, 150 2020. doi:10.3847/1538-4357/aad37d1a
NLM
Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
Vancouver
Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
Artigo de periodico
The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey (2019)
Placco, Vinicius M; Santucci, Rafael M; Rossi, Silvia Cristina Fernandes
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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PLACCO, Vinicius M e SANTUCCI, Rafael M e ROSSI, Silvia Cristina Fernandes. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, v. 870, n. 2, p. 122-1/122-11, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf3b9. Acesso em: 10 nov. 2024.
APA
Placco, V. M., Santucci, R. M., & Rossi, S. C. F. (2019). The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, 870( 2), 122-1/122-11. doi:10.3847/1538-4357/aaf3b9
NLM
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
Vancouver
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
Artigo de periodico
The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region (2018)
Galli, Phillip A. B; Loinard, Laurent; Otiz-Leon, Gisela N; Teixeira, Ramachrisna
Source: Astrophysical Journal. Unidade: IAG
Subjects: ASTROMETRIA, ESTRELAS BINÁRIAS
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GALLI, Phillip A. B et al. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region. Astrophysical Journal, v. 859, p. 33, 2018Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf. Acesso em: 10 nov. 2024.
APA
Galli, P. A. B., Loinard, L., Otiz-Leon, G. N., & Teixeira, R. (2018). The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region. Astrophysical Journal, 859, 33. doi:10.3847/1538-4357/aabf91
NLM
Galli PAB, Loinard L, Otiz-Leon GN, Teixeira R. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region [Internet]. Astrophysical Journal. 2018 ; 859 33.[citado 2024 nov. 10 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf
Vancouver
Galli PAB, Loinard L, Otiz-Leon GN, Teixeira R. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region [Internet]. Astrophysical Journal. 2018 ; 859 33.[citado 2024 nov. 10 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf
Artigo de periodico
Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres (2018)
Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Casey, Andrew R; Karakas, Amanda I; Tucci-Maia, Marcelo
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 10 nov. 2024.
APA
Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
NLM
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad190
Vancouver
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad190
Artigo de periodico
The chemical homogeneity of sun-like stars in the solar neighborhood (2018)
Bedell, Megan; Bean, Jacob L; Moreno, Jorge Luis Meléndez; Spina, Lorenzo; Ramirez, Ivan; Asplund, Martin; Alves-Brito, Alan; Santos, Leonardo dos; Dreizler, Stefan; Yong, David; Monroe, TalaWanda; Casagrande, Luca
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES
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ABNT
BEDELL, Megan et al. The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, v. 865, n. 1, p. 68-1/68-13, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 10 nov. 2024.
APA
Bedell, M., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., Asplund, M., et al. (2018). The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, 865( 1), 68-1/68-13. doi:10.3847/1538-4357/aad908
NLM
Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Vancouver
Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Artigo de periodico
Double nuclei in NGC 908 and NGC 1187 (2018)
Menezes, R. B; Steiner, João Evangelista
Source: Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS
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ABNT
MENEZES, R. B e STEINER, João Evangelista. Double nuclei in NGC 908 and NGC 1187. Astrophysical Journal, v. 868, p. 67, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aae843. Acesso em: 10 nov. 2024.
APA
Menezes, R. B., & Steiner, J. E. (2018). Double nuclei in NGC 908 and NGC 1187. Astrophysical Journal, 868, 67. doi:10.3847/1538-4357/aae843
NLM
Menezes RB, Steiner JE. Double nuclei in NGC 908 and NGC 1187 [Internet]. Astrophysical Journal. 2018 ; 868 67.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aae843
Vancouver
Menezes RB, Steiner JE. Double nuclei in NGC 908 and NGC 1187 [Internet]. Astrophysical Journal. 2018 ; 868 67.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aae843
Artigo de periodico
The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters (2018)
Chojnowski, S. Drew; Labadie-Bartz, Jonathan; Rivinius, Thomas; Gies, Douglas; Leister, Nelson Vani
Source: Astrophysical Journal. Unidade: IAG
Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CHOJNOWSKI, S. Drew et al. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, v. 865, n. 1, p. 76-1/76-16, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad964. Acesso em: 10 nov. 2024.
APA
Chojnowski, S. D., Labadie-Bartz, J., Rivinius, T., Gies, D., & Leister, N. V. (2018). The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, 865( 1), 76-1/76-16. doi:10.3847/1538-4357/aad964
NLM
Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad964
Vancouver
Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad964
Artigo de periodico
A formation timescale of the galactic Halo from Mg isotopes in dwarf stars (2018)
Carlos, Marília; Karakas, Amanda I; Cohen, Judith G; Kobayashi, Chiaki; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 10 nov. 2024.
APA
Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
NLM
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Vancouver
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Artigo de periodico
The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild (2018)
Cain, Madelyn; Frebel, Anna; Gull, Maude; Ji, Alexander P; Placco, Vinicius M; Beers, Timothy C; Moreno, Jorge Luis Meléndez; Ezzeddine, Rana; Casey, Andrew R; Hansen, Terese T; Roederer, Ian U; Sakari, Charli
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CAIN, Madelyn et al. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, v. 864, n. 1, p. 43-1/43-12, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 10 nov. 2024.
APA
Cain, M., Frebel, A., Gull, M., Ji, A. P., Placco, V. M., Beers, T. C., et al. (2018). The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, 864( 1), 43-1/43-12. doi:10.3847/1538-4357/aad37d
NLM
Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Vancouver
Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection (2018)
Kadowaki, Luis H. S; Dal Pino, Elisabete Maria de Gouveia; Stone, James M
Source: Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
KADOWAKI, Luis H. S e DAL PINO, Elisabete Maria de Gouveia e STONE, James M. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection. Astrophysical Journal, v. 864, n. 1, p. 52-1/52-17, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad4ff. Acesso em: 10 nov. 2024.
APA
Kadowaki, L. H. S., Dal Pino, E. M. de G., & Stone, J. M. (2018). MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection. Astrophysical Journal, 864( 1), 52-1/52-17. doi:10.3847/1538-4357/aad4ff
NLM
Kadowaki LHS, Dal Pino EM de G, Stone JM. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection [Internet]. Astrophysical Journal. 2018 ; 864( 1): 52-1/52-17.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad4ff
Vancouver
Kadowaki LHS, Dal Pino EM de G, Stone JM. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection [Internet]. Astrophysical Journal. 2018 ; 864( 1): 52-1/52-17.[citado 2024 nov. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad4ff

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