Study of the transient nature of classical Be stars using multi-epoch optical spectroscopy
Gourav Banerjee, Blesson Mathew, K. T. Paul, Annapurni Subramaniam,, Anjusha Balan, Suman Bhattacharyya, R. Anusha, Deeja Moosa, C S Dheeraj,, Aleeda Charly, Megha Raghu

TL;DR
This study monitors nine classical Be stars over five years to analyze their disc-loss and formation episodes through Hα line profile variations, revealing transient disc behaviors and timescales of disc evolution.
Contribution
It provides a detailed multi-epoch spectroscopic analysis of Be star disc variability, identifying phases of disc loss, formation, and stability over several years.
Findings
Four stars are undergoing disc-loss episodes.
One star is likely forming a new disc.
Four stars have stable discs in recent observations.
Abstract
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, complete disappearance of the H{\alpha} emission line occurs, indicating a disc-less state in CBe stars. The disc-loss and reappearing phases can be identified by studying the H{\alpha} line profiles of CBe stars on a regular basis. In this paper, we present the study of a set of selected 9 bright CBe stars, in the wavelength range of 6200 - 6700 {\AA}, to better understand their disc transient nature through continuous monitoring of their H{\alpha} line profile variations for 5 consecutive years (2015 -- 2019). Based on our observations, we suggest that 4 of the program stars (HD 4180, HD 142926, HD 164447 and HD 171780) are possibly undergoing disc-loss episodes, whereas one other star (HD 23302) might be passing through disc formation phase. The remaining 4 stars (HD 237056, HD 33357, HD…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Phase Equilibria and Thermodynamics
