Speaker
Mrs
Faide Huseynova
(Batabat Astrophysical Observatory, Nahkchivan State University)
Description
The results of spectral and photometric analyses of six chosen massive Herbig AeBe stars for the years 2023–2024 are presented in this research. Spectral investigations show that the emission spectra varies significantly across time intervals between one month and one year. The circumstellar disk's condition was described by an energy distribution curve. Two of the six stars are seen to have evolved debris disks with weak residual dust radiation. The stars' primary physical characteristics were computed, and their evolutionary status was determined. Due to its binarity, MWC 300 is a more developed star with significant excess infrared radiation.
| Stream | Science or Engineering |
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Primary author
Mrs
Faide Huseynova
(Batabat Astrophysical Observatory, Nahkchivan State University)
Co-authors
Prof.
Nariman İsmailov
(Tusi Shamakhy Astrophysical Observatory, Ministry of Science and Education of Azerbaijan)
Mr
Ulvu Valiyev
(Batabat Astrophysical Observatory, Nakhchivan State University)