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Ciencias Astronómicas
4
Circumstellar matter
4
Supergiants
3
Astronomía
2
Infrared: stars
2
Stars: emission line, Be
2
Stars: winds, outflows
2
circumstellar matter
2
stars: early-type
2
Be
1
Ciencias Exactas
1
Ciencias Naturales
1
Early-type emission stars
1
Física
1
Outflows
1
Stars: emission-line
1
Stars: individual: LHA115-S 65
1
Stars: massive
1
Stars: winds
1
infrared: stars
1
stars: emission-line Be
1
stars: individual (MWC 137)
1
stars: massive
1
supergiants
1
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1por Oksala, M. E., Kraus, M., Arias, María Laura, Borges Fernandes, M., Cidale, Lydia Sonia, Muratore, María Florencia, Curé, M.“... evolved massive stars, indicates an evolutionary link between B[e] supergiants and luminous blue variables....”
Publicado 2012
Aportado por: SEDICI (UNLP)Articulo -
2por Kraus, M., Cidale, Lydia Sonia, Arias, María Laura, Oksala, M.E., Borges Fernandes, M.“... calculations. However, B[e]SGs are not easily identified, as they share many characteristics with luminous blue...”
Publicado 2014
Aportado por: SEDICI (UNLP)Articulo -
3por Kourniotis, M., Kraus, M., Arias, María Laura, Cidale, Lydia Sonia, Torres, Andrea Fabiana“... the composition and geometry of their ejecta alongside the stellar properties. We selected five hot luminous blue...”
Publicado 2018
Aportado por: SEDICI (UNLP)Articulo Preprint -
4por Muratore, María Florencia, Kraus, M., Oksala, M. E., Arias, María Laura, Cidale, Lydia Sonia, Borges Fernandes, M., Liermann, A.“... that MWC 137 could be in an extremely short-lived phase, evolving from a B[e] supergiant to a blue...”
Publicado 2015
Aportado por: SEDICI (UNLP)Articulo -
5por Cochetti, Yanina Roxana, Kraus, Michaela, Arias, María Laura, Cidale, Lydia Sonia, Eenmäe, Tõnis, Liimets, T., Torres, Andrea Fabiana, Djupvik, A. A.“... show characteristics typically seen in Luminous Blue Variable (LBV) stars. In addition, we propose...”
Publicado 2020
Aportado por: SEDICI (UNLP)Articulo -
6por Liermann, A., Schnurr, O., Kraus, M., Kreplin, A., Arias, María Laura, Cidale, Lydia Sonia“... be characterized as evolved objects. Among others we find one luminous blue variable candidate (MWC314), one...”
Publicado 2014
Aportado por: SEDICI (UNLP)Articulo