Photometric and spectroscopic variations of the Be star HD 112999
Reviewed by Pithpith:BTKU5NONopen to challenge →
classification
astro-ph.SR
keywords
spectroscopicstarslinesphotometricstartransienttypeanalysis
read the original abstract
Be objects are stars of B spectral type showing lines of the Balmer series in emission. The presence of these lines is attributed to the existence of an extended envelope, disk type, around them. Some stars are observed in both the Be and normal B-type spectroscopic states and they are known as transient Be stars. In this paper we show the analysis carried out on a new possible transient Be star, labelled HD 112999, using spectroscopic optical observations and photometric data.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.