Speaker
CHIEN-DE LEE
(National Central University-Taiwan)
Description
B[e] stars are the hot stars with forbidden lines in their spectra, which can be found in a wide range of stellar ages, from pre-main sequence objects to evolved stars. However, the evolution of most objects with B[e] phenomena are yet to be classified. We study a sample of eight B[e] stars with uncertain evolutionary status to shed light on the origin of their circumstellar dust. We performed a diagnostic analysis on the spectral energy distribution beyond infrared wavelengths, and conducted a census of neighboring region of each target to ascertain its evolutionary status.
Primary author
CHIEN-DE LEE
(National Central University-Taiwan)
Co-authors
Sheng-Yuan Liu
(Institute of Astronomy and Astrophysics, Academia Sinica)
Wen-Ping Chen
(Graduate Institute of Astronomy, National Central University)
