Photometric and spectroscopic variability of the B5IIIe star HD 171219
We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type, whose spectra show, or have shown at some epoch, Balmer lines in emission and an infrared excess
Gutiérrez-Soto, J. et al.
Fecha de publicación:
7
2017