Source: The Astrophysical Journal. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS, ESTRELAS VARIÁVEIS, PERDA DE MASSA
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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: 07 set. 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 set. 07 ]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 set. 07 ]