R Coronae Borealis (RCB) stars are rare, and their evolutionary origin is not well understood. Since they are obscured due to formation of carbon dust around the star during their mass loss events, RCB stars can be classified as self-eclipsing variable stars. The purpose of this work is to present a new search for RCB stars in the Small Magellanic Cloud (SMC), by analysing VI data from the OGLE project....
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Autor | Nikzat, Fatemeh Catelan , Marcio |
Título | A new search for R Coronae Borealis stars in the SMC |
Fecha de publicación | 2017 |
Resumen | R Coronae Borealis (RCB) stars are rare, and their evolutionary origin is not well understood. Since they are obscured due to formation of carbon dust around the star during their mass loss events, RCB stars can be classified as self-eclipsing variable stars. The purpose of this work is to present a new search for RCB stars in the Small Magellanic Cloud (SMC), by analysing VI data from the OGLE project.... |
Derechos | acceso abierto |
DOI | 10.1051/epjconf/201715201020 |
Enlace | |
Id de publicación en WoS | WOS:000426610100020 |
Tipo de documento | comunicación de congreso |