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Artigo de periodico
Galactic transient sources with the Cherenkov Telescope Array Observatory (2025)
Abe, Koya; Pereira, Luiz Augusto Stuani ; Almeida, Ulisses Barres de ; Dal Pino, Elisabete Maria de Gouveia ; Souza, Vitor de ; del Valle, Maria Victoria; Gonçalves, Diego Antonio Falceta ; Kowal, Grzegorz ; Silva, Rodrigo Nemmen da ; Reis, Igor ; Viana, Aion
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IFSC, EACH
Subjects: RAIOS X, RAIOS CÓSMICOS, ASTROFÍSICA, OBSERVATÓRIOS
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ABNT
ABE, Koya et al. Galactic transient sources with the Cherenkov Telescope Array Observatory. Monthly Notices of the Royal Astronomical Society, v. 540, n. 1, p. 205-238, 2025Tradução . . Disponível em: https://doi.org/10.1093/mnras/staf655. Acesso em: 01 dez. 2025.
APA
Abe, K., Pereira, L. A. S., Almeida, U. B. de, Dal Pino, E. M. de G., Souza, V. de, del Valle, M. V., et al. (2025). Galactic transient sources with the Cherenkov Telescope Array Observatory. Monthly Notices of the Royal Astronomical Society, 540( 1), 205-238. doi:10.1093/mnras/staf655
NLM
Abe K, Pereira LAS, Almeida UB de, Dal Pino EM de G, Souza V de, del Valle MV, Gonçalves DAF, Kowal G, Silva RN da, Reis I, Viana A. Galactic transient sources with the Cherenkov Telescope Array Observatory [Internet]. Monthly Notices of the Royal Astronomical Society. 2025 ; 540( 1): 205-238.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/staf655
Vancouver
Abe K, Pereira LAS, Almeida UB de, Dal Pino EM de G, Souza V de, del Valle MV, Gonçalves DAF, Kowal G, Silva RN da, Reis I, Viana A. Galactic transient sources with the Cherenkov Telescope Array Observatory [Internet]. Monthly Notices of the Royal Astronomical Society. 2025 ; 540( 1): 205-238.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/staf655
Artigo de periodico
Diffusion of large-scale magnetic fields by reconnection in MHD turbulence (2021)
Santos-Lima, R ; Guerrero, G; Dal Pino, Elisabete Maria de Gouveia ; Lazarian, A.
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assunto: CAMPO MAGNÉTICO
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SANTOS-LIMA, R et al. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, v. 503, p. 1290-1309, 2021Tradução . . Disponível em: https://academic.oup.com/mnras/article/503/1/1290/6144594. Acesso em: 01 dez. 2025.
APA
Santos-Lima, R., Guerrero, G., Dal Pino, E. M. de G., & Lazarian, A. (2021). Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, 503, 1290-1309. doi:10.1093/mnras/stab470
NLM
Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2025 dez. 01 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
Vancouver
Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2025 dez. 01 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
Artigo de periodico
The impact of plasma instabilities on the spectra of TeV blazars (2019)
Batista, Rafael Alves; Saveliev, Andrey; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, RAIOS GAMA
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BATISTA, Rafael Alves e SAVELIEV, Andrey e DAL PINO, Elisabete Maria de Gouveia. The impact of plasma instabilities on the spectra of TeV blazars. Monthly Notices of the Royal Astronomical Society, v. 489, n. 3, p. 3836-3849, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2389. Acesso em: 01 dez. 2025.
APA
Batista, R. A., Saveliev, A., & Dal Pino, E. M. de G. (2019). The impact of plasma instabilities on the spectra of TeV blazars. Monthly Notices of the Royal Astronomical Society, 489( 3), 3836-3849. doi:10.1093/mnras/stz2389
NLM
Batista RA, Saveliev A, Dal Pino EM de G. The impact of plasma instabilities on the spectra of TeV blazars [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 3): 3836-3849.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stz2389
Vancouver
Batista RA, Saveliev A, Dal Pino EM de G. The impact of plasma instabilities on the spectra of TeV blazars [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 3): 3836-3849.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stz2389
Artigo de periodico
Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts (2019)
Barai, Paramita; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: BURACOS NEGROS, HIDRODINÂMICA, QUASARES, ESTRUTURA DO UNIVERSO
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ABNT
BARAI, Paramita e DAL PINO, Elisabete Maria de Gouveia. Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts. Monthly Notices of the Royal Astronomical Society, v. 487, n. 4, p. 5549-5563, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz1616. Acesso em: 01 dez. 2025.
APA
Barai, P., & Dal Pino, E. M. de G. (2019). Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts. Monthly Notices of the Royal Astronomical Society, 487( 4), 5549-5563. doi:10.1093/mnras/stz1616
NLM
Barai P, Dal Pino EM de G. Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 487( 4): 5549-5563.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stz1616
Vancouver
Barai P, Dal Pino EM de G. Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 487( 4): 5549-5563.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stz1616
Artigo de periodico
Magnetic reconnection and Blandford–Znajek process around rotating black holes (2018)
Singh, Chandra B; Garofalo, David; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, BURACOS NEGROS, RAIOS X
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ABNT
SINGH, Chandra B e GAROFALO, David e DAL PINO, Elisabete Maria de Gouveia. Magnetic reconnection and Blandford–Znajek process around rotating black holes. Monthly Notices of the Royal Astronomical Society, v. 478, n. 4, p. 5404-5409, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1405. Acesso em: 01 dez. 2025.
APA
Singh, C. B., Garofalo, D., & Dal Pino, E. M. de G. (2018). Magnetic reconnection and Blandford–Znajek process around rotating black holes. Monthly Notices of the Royal Astronomical Society, 478( 4), 5404-5409. doi:10.1093/mnras/sty1405
NLM
Singh CB, Garofalo D, Dal Pino EM de G. Magnetic reconnection and Blandford–Znajek process around rotating black holes [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 478( 4): 5404-5409.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sty1405
Vancouver
Singh CB, Garofalo D, Dal Pino EM de G. Magnetic reconnection and Blandford–Znajek process around rotating black holes [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 478( 4): 5404-5409.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sty1405
Artigo de periodico
The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays (2018)
Kushwaha, Pankaj; Gupta, Alok C; Wiita, Paul J; Pal, Main; Gaur, Haritma; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assunto: RAIOS X
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ABNT
KUSHWAHA, Pankaj et al. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays. Monthly Notices of the Royal Astronomical Society, v. 479, p. 1672-1684, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1499. Acesso em: 01 dez. 2025.
APA
Kushwaha, P., Gupta, A. C., Wiita, P. J., Pal, M., Gaur, H., & Dal Pino, E. M. de G. (2018). The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays. Monthly Notices of the Royal Astronomical Society, 479, 1672-1684. doi:10.1093/mnras/sty1499
NLM
Kushwaha P, Gupta AC, Wiita PJ, Pal M, Gaur H, Dal Pino EM de G. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 1672-1684.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sty1499
Vancouver
Kushwaha P, Gupta AC, Wiita PJ, Pal M, Gaur H, Dal Pino EM de G. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 1672-1684.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sty1499
Artigo de periodico
Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback (2017)
Santos-Lima, Reinaldo; Dal Pino, Elisabete Maria de Gouveia; Gonçalves, Diego Antonio Falceta ; Nakwacki, Maria Soledad; Kowal, Grzegorz
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Subjects: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS, MEIO INTERESTELAR
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ABNT
SANTOS-LIMA, Reinaldo et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, v. 465, n. 4, p. 4866-4871, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw3050. Acesso em: 01 dez. 2025.
APA
Santos-Lima, R., Dal Pino, E. M. de G., Gonçalves, D. A. F., Nakwacki, M. S., & Kowal, G. (2017). Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, 465( 4), 4866-4871. doi:10.1093/mnras/stw3050
NLM
Santos-Lima R, Dal Pino EM de G, Gonçalves DAF, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stw3050
Vancouver
Santos-Lima R, Dal Pino EM de G, Gonçalves DAF, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stw3050
Artigo de periodico
Properties of the First-order Fermi acceleration in fast magnetic reconnection driven by turbulence in collisional magnetohydrodynamical flows (2016)
del Valle, Maria Victoria; Dal Pino, Elisabete Maria de Gouveia; Kowal, Grzegorz
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ACELERADOR DE PARTÍCULAS, ASTROFÍSICA ESTELAR
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ABNT
DEL VALLE, Maria Victoria e DAL PINO, Elisabete Maria de Gouveia e KOWAL, Grzegorz. Properties of the First-order Fermi acceleration in fast magnetic reconnection driven by turbulence in collisional magnetohydrodynamical flows. Monthly Notices of the Royal Astronomical Society, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1609.08598.pdf. Acesso em: 01 dez. 2025.
APA
del Valle, M. V., Dal Pino, E. M. de G., & Kowal, G. (2016). Properties of the First-order Fermi acceleration in fast magnetic reconnection driven by turbulence in collisional magnetohydrodynamical flows. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/STW2276
NLM
del Valle MV, Dal Pino EM de G, Kowal G. Properties of the First-order Fermi acceleration in fast magnetic reconnection driven by turbulence in collisional magnetohydrodynamical flows [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2025 dez. 01 ] Available from: https://arxiv.org/pdf/1609.08598.pdf
Vancouver
del Valle MV, Dal Pino EM de G, Kowal G. Properties of the First-order Fermi acceleration in fast magnetic reconnection driven by turbulence in collisional magnetohydrodynamical flows [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2025 dez. 01 ] Available from: https://arxiv.org/pdf/1609.08598.pdf
Artigo de periodico
High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration (2016)
Khiali, B; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ACELERAÇÃO DE PARTÍCULAS, NEUTRINOS, RADIAÇÃO NÃO TÉRMICA, MAGNETOHIDRODINÂMICA
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ABNT
KHIALI, B e DAL PINO, Elisabete Maria de Gouveia. High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration. Monthly Notices of the Royal Astronomical Society, v. 455, p. 838-845, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2337. Acesso em: 01 dez. 2025.
APA
Khiali, B., & Dal Pino, E. M. de G. (2016). High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration. Monthly Notices of the Royal Astronomical Society, 455, 838-845. doi:10.1093/mnras/stv2337
NLM
Khiali B, Dal Pino EM de G. High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455 838-845.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stv2337
Vancouver
Khiali B, Dal Pino EM de G. High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455 838-845.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stv2337
Artigo de periodico
Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps (2016)
Nakwacki, Maria Soledad; Kowal, Grzegorz ; Santos-Lima, Reinaldo; Dal Pino, Elisabete Maria de Gouveia; Gonçalves, Diego Antonio Falceta
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Subjects: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS
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ABNT
NAKWACKI, Maria Soledad et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, v. 455, n. 4, p. 3702-3723, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2586. Acesso em: 01 dez. 2025.
APA
Nakwacki, M. S., Kowal, G., Santos-Lima, R., Dal Pino, E. M. de G., & Gonçalves, D. A. F. (2016). Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, 455( 4), 3702-3723. doi:10.1093/mnras/stv2586
NLM
Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Gonçalves DAF. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stv2586
Vancouver
Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Gonçalves DAF. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stv2586
Artigo de periodico
Limits on the ions temperature anisotropy in turbulent intracluster medium (2016)
Santos-Lima, R; Yan, H; Dal Pino, Elisabete Maria de Gouveia; Lazarian, A
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: MAGNETOHIDRODINÂMICA, PLASMA, TURBULÊNCIA, AGLOMERADOS DE GALÁXIAS
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ABNT
SANTOS-LIMA, R et al. Limits on the ions temperature anisotropy in turbulent intracluster medium. Monthly Notices of the Royal Astronomical Society, v. 460, p. 2492-2504, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw1079. Acesso em: 01 dez. 2025.
APA
Santos-Lima, R., Yan, H., Dal Pino, E. M. de G., & Lazarian, A. (2016). Limits on the ions temperature anisotropy in turbulent intracluster medium. Monthly Notices of the Royal Astronomical Society, 460, 2492-2504. doi:10.1093/mnras/stw1079
NLM
Santos-Lima R, Yan H, Dal Pino EM de G, Lazarian A. Limits on the ions temperature anisotropy in turbulent intracluster medium [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 460 2492-2504.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stw1079
Vancouver
Santos-Lima R, Yan H, Dal Pino EM de G, Lazarian A. Limits on the ions temperature anisotropy in turbulent intracluster medium [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 460 2492-2504.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stw1079
Artigo de periodico
Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? (2013)
Santos-Lima, R; Dal Pino, Elisabete Maria de Gouveia; Lazarian, A
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, TURBULÊNCIA, MEIO INTERESTELAR, CAMPO MAGNÉTICO
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ABNT
SANTOS-LIMA, R e DAL PINO, Elisabete Maria de Gouveia e LAZARIAN, A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?. Monthly Notices of the Royal Astronomical Society, v. 429. p. 3371-3378, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/sts597. Acesso em: 01 dez. 2025.
APA
Santos-Lima, R., Dal Pino, E. M. de G., & Lazarian, A. (2013). Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? Monthly Notices of the Royal Astronomical Society, 429. p. 3371-3378. doi:10.1093/mnras/sts597
NLM
Santos-Lima R, Dal Pino EM de G, Lazarian A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429. p. 3371-3378[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sts597
Vancouver
Santos-Lima R, Dal Pino EM de G, Lazarian A. Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not? [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429. p. 3371-3378[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/sts597
Artigo de periodico
Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations (2013)
Melioli, C; Dal Pino, Elisabete Maria de Gouveia; Geraissate, F. G
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: MEIO INTERESTELAR, ABUNDÂNCIAS (ASTRONOMIA), JATOS (ASTRONOMIA), GALÁXIAS
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ABNT
MELIOLI, C e DAL PINO, Elisabete Maria de Gouveia e GERAISSATE, F. G. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, v. 430, p. 3235-3248, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt126. Acesso em: 01 dez. 2025.
APA
Melioli, C., Dal Pino, E. M. de G., & Geraissate, F. G. (2013). Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, 430, 3235-3248. doi:10.1093/mnras/stt126
NLM
Melioli C, Dal Pino EM de G, Geraissate FG. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 430 3235-3248.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stt126
Vancouver
Melioli C, Dal Pino EM de G, Geraissate FG. Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 430 3235-3248.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1093/mnras/stt126
Artigo de periodico
Hydrodynamical simulations of Galactic fountains: II. Evolution of multiple fountains (2009)
Melioli, C; Dal Pino, Elisabete Maria de Gouveia; Brighenti, F; D`Ercole, A
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: HIDRODINÂMICA, MÉTODOS NUMÉRICOS, MEIO INTERESTELAR, NUVENS, GALÁXIAS
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ABNT
MELIOLI, C et al. Hydrodynamical simulations of Galactic fountains: II. Evolution of multiple fountains. Monthly Notices of the Royal Astronomical Society, v. 399, p. 1089-1105, 2009Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2009.14725.x. Acesso em: 01 dez. 2025.
APA
Melioli, C., Dal Pino, E. M. de G., Brighenti, F., & D`Ercole, A. (2009). Hydrodynamical simulations of Galactic fountains: II. Evolution of multiple fountains. Monthly Notices of the Royal Astronomical Society, 399, 1089-1105. doi:10.1111/j.1365-2966.2009.14725.x
NLM
Melioli C, Dal Pino EM de G, Brighenti F, D`Ercole A. Hydrodynamical simulations of Galactic fountains: II. Evolution of multiple fountains [Internet]. Monthly Notices of the Royal Astronomical Society. 2009 ; 399 1089-1105.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1111/j.1365-2966.2009.14725.x
Vancouver
Melioli C, Dal Pino EM de G, Brighenti F, D`Ercole A. Hydrodynamical simulations of Galactic fountains: II. Evolution of multiple fountains [Internet]. Monthly Notices of the Royal Astronomical Society. 2009 ; 399 1089-1105.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1111/j.1365-2966.2009.14725.x
Artigo de periodico
Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds (2009)
Leão, M.R.M; Dal Pino, Elisabete Maria de Gouveia; Gonçalves, Diego Antonio Falceta ; Melioli, C; Geraissate, F. G
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: FORMAÇÃO DE ESTRELAS, MEIO INTERESTELAR, SUPERNOVAS, NUVENS
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ABNT
LEÃO, M.R.M et al. Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds. Monthly Notices of the Royal Astronomical Society, v. 394, p. 157-173, 2009Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2008.14337.x. Acesso em: 01 dez. 2025.
APA
Leão, M. R. M., Dal Pino, E. M. de G., Gonçalves, D. A. F., Melioli, C., & Geraissate, F. G. (2009). Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds. Monthly Notices of the Royal Astronomical Society, 394, 157-173. doi:10.1111/j.1365-2966.2008.14337.x
NLM
Leão MRM, Dal Pino EM de G, Gonçalves DAF, Melioli C, Geraissate FG. Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds [Internet]. Monthly Notices of the Royal Astronomical Society. 2009 ; 394 157-173.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.14337.x
Vancouver
Leão MRM, Dal Pino EM de G, Gonçalves DAF, Melioli C, Geraissate FG. Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds [Internet]. Monthly Notices of the Royal Astronomical Society. 2009 ; 394 157-173.[citado 2025 dez. 01 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.14337.x

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