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Artigo de periodico
Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid (2022)
Razera, R ; Barbuy, Beatriz Leonor Silveira ; Moura, T. C ; Ernandes, H ; Friaça, Amâncio César Santos
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IF
Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
RAZERA, R et al. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, v. 517, p. 4590-4606, 2022Tradução . . Disponível em: https://academic.oup.com/mnras/article/517/3/4590/6653110. Acesso em: 11 out. 2024.
APA
Razera, R., Barbuy, B. L. S., Moura, T. C., Ernandes, H., & Friaça, A. C. S. (2022). Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, 517, 4590-4606. doi:10.1093/mnras/stac2136
NLM
Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 out. 11 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
Vancouver
Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 out. 11 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
Artigo de periodico
Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy (2022)
Ernandes, H ; Barbuy, Beatriz Leonor Silveira ; Friaça, Amâncio César Santos; Hill, V; Spite, M; Spite, F; Castilho, B. V; Evans, C. J
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
ERNANDES, H et al. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, v. 510, p. 5362-5375, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3789. Acesso em: 11 out. 2024.
APA
Ernandes, H., Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Spite, M., Spite, F., et al. (2022). Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, 510, 5362-5375. doi:10.1093/mnras/stab3789
NLM
Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stab3789
Vancouver
Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stab3789
Artigo de periodico
The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle (2016)
Gull, Theodore R; Madura, Thomas I; Teodoro, Mairan; Clementel, Nicola; Corcoran, Michael; Damineli Neto, Augusto; Groh, Jose H; Hamaguchi, Kenji; Hillier, D. John; Moffat, Anthony F. J; Richardson, Noel D; Weigelt, Gerd; Lindler, Don; Feggans, Keith
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS, PERDA DE MASSA, ESTRELAS VARIÁVEIS
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ABNT
GULL, Theodore R et al. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle. Monthly Notices of the Royal Astronomical Society, v. 462, p. 3196-3220, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw1829. Acesso em: 11 out. 2024.
APA
Gull, T. R., Madura, T. I., Teodoro, M., Clementel, N., Corcoran, M., Damineli Neto, A., et al. (2016). The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle. Monthly Notices of the Royal Astronomical Society, 462, 3196-3220. doi:10.1093/mnras/stw1829
NLM
Gull TR, Madura TI, Teodoro M, Clementel N, Corcoran M, Damineli Neto A, Groh JH, Hamaguchi K, Hillier DJ, Moffat AFJ, Richardson ND, Weigelt G, Lindler D, Feggans K. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3196-3220.[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stw1829
Vancouver
Gull TR, Madura TI, Teodoro M, Clementel N, Corcoran M, Damineli Neto A, Groh JH, Hamaguchi K, Hillier DJ, Moffat AFJ, Richardson ND, Weigelt G, Lindler D, Feggans K. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3196-3220.[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stw1829
Artigo de periodico
UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 (2014)
Keller, Graziela R; Bianchi, Luciana; Maciel, Walter Junqueira
Source: Monthly Notices Royal Astronomical Society. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES, PERDA DE MASSA, VENTO
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ABNT
KELLER, Graziela R e BIANCHI, Luciana e MACIEL, Walter Junqueira. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3. Monthly Notices Royal Astronomical Society, v. 442, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu878. Acesso em: 11 out. 2024.
APA
Keller, G. R., Bianchi, L., & Maciel, W. J. (2014). UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3. Monthly Notices Royal Astronomical Society, 442. doi:10.1093/mnras/stu878
NLM
Keller GR, Bianchi L, Maciel WJ. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 [Internet]. Monthly Notices Royal Astronomical Society. 2014 ; 442[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stu878
Vancouver
Keller GR, Bianchi L, Maciel WJ. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 [Internet]. Monthly Notices Royal Astronomical Society. 2014 ; 442[citado 2024 out. 11 ] Available from: https://doi.org/10.1093/mnras/stu878
Artigo de periodico
Heavy elements in old very metal-rich stars (2014)
Trevisan, M; Barbuy, Beatriz Leonor Silveira
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, SOL
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ABNT
TREVISAN, M e BARBUY, Beatriz Leonor Silveira. Heavy elements in old very metal-rich stars. Astronomy & Astrophysics, v. 570, p. A22/1-A22/13, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322967. Acesso em: 11 out. 2024.
APA
Trevisan, M., & Barbuy, B. L. S. (2014). Heavy elements in old very metal-rich stars. Astronomy & Astrophysics, 570, A22/1-A22/13. doi:10.1051/0004-6361/201322967
NLM
Trevisan M, Barbuy BLS. Heavy elements in old very metal-rich stars [Internet]. Astronomy & Astrophysics. 2014 ; 570 A22/1-A22/13.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201322967
Vancouver
Trevisan M, Barbuy BLS. Heavy elements in old very metal-rich stars [Internet]. Astronomy & Astrophysics. 2014 ; 570 A22/1-A22/13.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201322967
Artigo de periodico
The future of the Sun: an evolved solar twin revealed by CoRoT (2013)
Nascimento Júnior, J.-D. do; Takeda, Y; Moreno, Jorge Luis Meléndez; Costa, J. S. da; Mello, G. F. Porto de; Castro, M
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, SOL
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ABNT
NASCIMENTO JÚNIOR, J.-D. do et al. The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, v. 771, p. L31/1-L31/5, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/771/2/L31. Acesso em: 11 out. 2024.
APA
Nascimento Júnior, J. -D. do, Takeda, Y., Moreno, J. L. M., Costa, J. S. da, Mello, G. F. P. de, & Castro, M. (2013). The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, 771, L31/1-L31/5. doi:10.1088/2041-8205/771/2/L31
NLM
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 out. 11 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
Vancouver
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 out. 11 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
Artigo de periodico
A study of accretion disk wind emission (2012)
Puebla, R. E; Diaz, Marcos Perez; Hillier, D.J.
Source: Memorie della Società Astronomica Italiana. Unidade: IAG
Subjects: ESTRELAS, DISCOS DE ACRESÇÃO, ATMOSFERAS ESTELARES, VENTO
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ABNT
PUEBLA, R. E e DIAZ, Marcos Perez e HILLIER, D.J. A study of accretion disk wind emission. Memorie della Società Astronomica Italiana, v. 83, p. 525-529, 2012Tradução . . Acesso em: 11 out. 2024.
APA
Puebla, R. E., Diaz, M. P., & Hillier, D. J. (2012). A study of accretion disk wind emission. Memorie della Società Astronomica Italiana, 83, 525-529.
NLM
Puebla RE, Diaz MP, Hillier DJ. A study of accretion disk wind emission. Memorie della Società Astronomica Italiana. 2012 ; 83 525-529.[citado 2024 out. 11 ]
Vancouver
Puebla RE, Diaz MP, Hillier DJ. A study of accretion disk wind emission. Memorie della Società Astronomica Italiana. 2012 ; 83 525-529.[citado 2024 out. 11 ]
Artigo de periodico
Reddenings of Cepheids (2012)
Andrievsky, S. M; Luck, R. E; Kovtyukh, V. V; Lepine, Jacques Raymond Daniel
Source: Publications of the Astronomical Society of the Pacific. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES, FOTOMETRIA
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ABNT
ANDRIEVSKY, S. M et al. Reddenings of Cepheids. Publications of the Astronomical Society of the Pacific, v. 124, p. 934-938, 2012Tradução . . Disponível em: https://doi.org/10.1086/668085. Acesso em: 11 out. 2024.
APA
Andrievsky, S. M., Luck, R. E., Kovtyukh, V. V., & Lepine, J. R. D. (2012). Reddenings of Cepheids. Publications of the Astronomical Society of the Pacific, 124, 934-938. doi:10.1086/668085
NLM
Andrievsky SM, Luck RE, Kovtyukh VV, Lepine JRD. Reddenings of Cepheids [Internet]. Publications of the Astronomical Society of the Pacific. 2012 ; 124 934-938.[citado 2024 out. 11 ] Available from: https://doi.org/10.1086/668085
Vancouver
Andrievsky SM, Luck RE, Kovtyukh VV, Lepine JRD. Reddenings of Cepheids [Internet]. Publications of the Astronomical Society of the Pacific. 2012 ; 124 934-938.[citado 2024 out. 11 ] Available from: https://doi.org/10.1086/668085
Artigo de periodico
Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars (2012)
Maciel, Walter Junqueira; Costa, Roberto Dell'Aglio Dias da
Source: Memorie della Società Astronomica Italiana. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, METAIS
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ABNT
MACIEL, Walter Junqueira e COSTA, Roberto Dell'Aglio Dias da. Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars. Memorie della Società Astronomica Italiana, v. 22, p. 103-109, 2012Tradução . . Acesso em: 11 out. 2024.
APA
Maciel, W. J., & Costa, R. D. 'A. D. da. (2012). Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars. Memorie della Società Astronomica Italiana, 22, 103-109.
NLM
Maciel WJ, Costa RD'AD da. Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars. Memorie della Società Astronomica Italiana. 2012 ; 22 103-109.[citado 2024 out. 11 ]
Vancouver
Maciel WJ, Costa RD'AD da. Littium abundances and metallicities: trends from metal-poor and AGB/RGB stars. Memorie della Società Astronomica Italiana. 2012 ; 22 103-109.[citado 2024 out. 11 ]
Artigo de periodico
Lithium in M 67: from the main sequence to the red giant branch (2012)
Pace, G; Castro, M; Meléndez Moreno, Jorge Luis; Théado, S; Nascimento Jr., J.-D do
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
PACE, G et al. Lithium in M 67: from the main sequence to the red giant branch. Astronomy & Astrophysics, v. 541, p. A150/1-A150/10, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201117704. Acesso em: 11 out. 2024.
APA
Pace, G., Castro, M., Meléndez Moreno, J. L., Théado, S., & Nascimento Jr., J. -D. do. (2012). Lithium in M 67: from the main sequence to the red giant branch. Astronomy & Astrophysics, 541, A150/1-A150/10. doi:10.1051/0004-6361/201117704
NLM
Pace G, Castro M, Meléndez Moreno JL, Théado S, Nascimento Jr. J-D do. Lithium in M 67: from the main sequence to the red giant branch [Internet]. Astronomy & Astrophysics. 2012 ; 541 A150/1-A150/10.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201117704
Vancouver
Pace G, Castro M, Meléndez Moreno JL, Théado S, Nascimento Jr. J-D do. Lithium in M 67: from the main sequence to the red giant branch [Internet]. Astronomy & Astrophysics. 2012 ; 541 A150/1-A150/10.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201117704
Artigo de periodico
Elemental abundances and classification of carbon-enhanced metal-poor stars (2012)
Allen, D. M; Ryan, S. G; Rossi, Sílvia Cristina Fernandes; Beers, T. C; Tsangarides, S. A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, ASTROQUÍMICA, CARBONO
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ABNT
ALLEN, D. M et al. Elemental abundances and classification of carbon-enhanced metal-poor stars. Astronomy & Astrophysics, v. 548, p. A34/1-A34/34, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201015615. Acesso em: 11 out. 2024.
APA
Allen, D. M., Ryan, S. G., Rossi, S. C. F., Beers, T. C., & Tsangarides, S. A. (2012). Elemental abundances and classification of carbon-enhanced metal-poor stars. Astronomy & Astrophysics, 548, A34/1-A34/34. doi:10.1051/0004-6361/201015615
NLM
Allen DM, Ryan SG, Rossi SCF, Beers TC, Tsangarides SA. Elemental abundances and classification of carbon-enhanced metal-poor stars [Internet]. Astronomy & Astrophysics. 2012 ; 548 A34/1-A34/34.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201015615
Vancouver
Allen DM, Ryan SG, Rossi SCF, Beers TC, Tsangarides SA. Elemental abundances and classification of carbon-enhanced metal-poor stars [Internet]. Astronomy & Astrophysics. 2012 ; 548 A34/1-A34/34.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201015615
Trabalho de evento
Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) (2012)
Keller, Graziela R; Bianchi, Luciana; Herald, James E; Maciel, Walter Junqueira
Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES, PERDA DE MASSA, VENTO
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ABNT
KELLER, Graziela R et al. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011647. Acesso em: 11 out. 2024.
APA
Keller, G. R., Bianchi, L., Herald, J. E., & Maciel, W. J. (2012). Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312011647
NLM
Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 11 ] Available from: https://doi.org/10.1017/S1743921312011647
Vancouver
Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 11 ] Available from: https://doi.org/10.1017/S1743921312011647
Trabalho de evento
FEROS abundance analysis of 21 bulgelike SMR stars (2010)
Trevisan, Marina; Barbuy, Beatriz Leonor Silveira; Grenon, M; Gustafsson, B; Pompéia, L
Source: Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Conference titles: IAU Symposium. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, ATMOSFERAS ESTELARES, GALÁXIAS
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ABNT
TREVISAN, Marina et al. FEROS abundance analysis of 21 bulgelike SMR stars. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 11 out. 2024.
APA
Trevisan, M., Barbuy, B. L. S., Grenon, M., Gustafsson, B., & Pompéia, L. (2010). FEROS abundance analysis of 21 bulgelike SMR stars. In Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Cambridge: Cambridge University Press.
NLM
Trevisan M, Barbuy BLS, Grenon M, Gustafsson B, Pompéia L. FEROS abundance analysis of 21 bulgelike SMR stars. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 out. 11 ]
Vancouver
Trevisan M, Barbuy BLS, Grenon M, Gustafsson B, Pompéia L. FEROS abundance analysis of 21 bulgelike SMR stars. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 out. 11 ]
Artigo de periodico
Detection of high-velocity material from the wind-wind collision zone of Eta Carinae across the 2009.0 periastron passage (2010)
Groh, J. H; Damineli Neto, Augusto; Teodoro, M
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES
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ABNT
GROH, J. H e DAMINELI NETO, Augusto e TEODORO, M. Detection of high-velocity material from the wind-wind collision zone of Eta Carinae across the 2009.0 periastron passage. Astronomy & Astrophysics, v. 517, p. A9/1-A9/17, 2010Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/200913937. Acesso em: 11 out. 2024.
APA
Groh, J. H., Damineli Neto, A., & Teodoro, M. (2010). Detection of high-velocity material from the wind-wind collision zone of Eta Carinae across the 2009.0 periastron passage. Astronomy & Astrophysics, 517, A9/1-A9/17. doi:10.1051/0004-6361/200913937
NLM
Groh JH, Damineli Neto A, Teodoro M. Detection of high-velocity material from the wind-wind collision zone of Eta Carinae across the 2009.0 periastron passage [Internet]. Astronomy & Astrophysics. 2010 ; 517 A9/1-A9/17.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/200913937
Vancouver
Groh JH, Damineli Neto A, Teodoro M. Detection of high-velocity material from the wind-wind collision zone of Eta Carinae across the 2009.0 periastron passage [Internet]. Astronomy & Astrophysics. 2010 ; 517 A9/1-A9/17.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/200913937
Artigo de periodico
Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae (2009)
Groh, J.H; Barbá, R; Damineli Neto, Augusto; Hillier, D.J; Fernández-Lajús; Gamen, R. C; Moisés, A. P; Solivella, G; Teodoro, M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS, ESTRELAS VARIÁVEIS, PERDA DE MASSA
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ABNT
GROH, J.H et al. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal, v. 705, p. L25-L30, 2009Tradução . . Acesso em: 11 out. 2024.
APA
Groh, J. H., Barbá, R., Damineli Neto, A., Hillier, D. J., Fernández-Lajús,, Gamen, R. C., et al. (2009). Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal, 705, L25-L30.
NLM
Groh JH, Barbá R, Damineli Neto A, Hillier DJ, Fernández-Lajús, Gamen RC, Moisés AP, Solivella G, Teodoro M. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal. 2009 ; 705 L25-L30.[citado 2024 out. 11 ]
Vancouver
Groh JH, Barbá R, Damineli Neto A, Hillier DJ, Fernández-Lajús, Gamen RC, Moisés AP, Solivella G, Teodoro M. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal. 2009 ; 705 L25-L30.[citado 2024 out. 11 ]
Artigo de periodico
On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle (2009)
Groh, J.H; Hiller, J. D; Damineli Neto, Augusto; Withelock, P. A; Marang, F; Rossi, C
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS, PERDA DE MASSA, ESTRELAS VARIÁVEIS
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ABNT
GROH, J.H et al. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal, v. 698, p. 1698-1720, 2009Tradução . . Acesso em: 11 out. 2024.
APA
Groh, J. H., Hiller, J. D., Damineli Neto, A., Withelock, P. A., Marang, F., & Rossi, C. (2009). On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal, 698, 1698-1720.
NLM
Groh JH, Hiller JD, Damineli Neto A, Withelock PA, Marang F, Rossi C. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal. 2009 ; 698 1698-1720.[citado 2024 out. 11 ]
Vancouver
Groh JH, Hiller JD, Damineli Neto A, Withelock PA, Marang F, Rossi C. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal. 2009 ; 698 1698-1720.[citado 2024 out. 11 ]
Artigo de periodico
AG Carinae: a luminous blue variable with a high rotational velocity (2006)
Groh, J. H; Hillier, D. J; Damineli Neto, Augusto
Source: Astrophysical Journal. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GROH, J. H e HILLIER, D. J e DAMINELI NETO, Augusto. AG Carinae: a luminous blue variable with a high rotational velocity. Astrophysical Journal, v. 638, p. L33-L36, 2006Tradução . . Acesso em: 11 out. 2024.
APA
Groh, J. H., Hillier, D. J., & Damineli Neto, A. (2006). AG Carinae: a luminous blue variable with a high rotational velocity. Astrophysical Journal, 638, L33-L36.
NLM
Groh JH, Hillier DJ, Damineli Neto A. AG Carinae: a luminous blue variable with a high rotational velocity. Astrophysical Journal. 2006 ; 638 L33-L36.[citado 2024 out. 11 ]
Vancouver
Groh JH, Hillier DJ, Damineli Neto A. AG Carinae: a luminous blue variable with a high rotational velocity. Astrophysical Journal. 2006 ; 638 L33-L36.[citado 2024 out. 11 ]

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