Autor:
Mehner, A.
Baade, D.
Groh, J.H.
Rivinius, T.
Hambsch, F.-J.
Bartlett, E.S.
Asmus, D.
Agliozzo, C.
Szeifert, T.
Stahl, O.
Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that are not yet understood. Stars can lose several solar masses during this evolutionary phase. The LBV phenomenon is thus critical to our understanding of the evolution of the most massive stars. Aims. ...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/6202
Mehner, A.
,
Baade, D.
,
Groh, J.H.
,
Rivinius, T.
,
Hambsch, F.-J.
,
Bartlett, E.S.
,
Asmus, D.
,
Agliozzo, C.
,
Szeifert, T.
,
Stahl, O.
,
[Spectroscopic and photometric oscillatory envelope variability during the S Doradus outburst of the luminous blue variable R71]
,
Spectroscopic and photometric oscillatory envelope variability during the S Doradus outburst of the luminous blue variable R71
