Searching for Accreting Compact Binary Systems from Spectroscopy and Photometry: Application to LAMOST Spectra

Compact objects undergoing mass transfer exhibit significant (and double-peaked) H _α emission lines. Recently, new methods have been developed to identify black hole X-ray binaries and calculate their systematic parameters using H _α line parameters, such as the full width at half-maximum (FWHM), e...

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Detalhes bibliográficos

Principais autores:	Xinlin Zhao, Song Wang, Jifeng Liu
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Binary stars Black holes Cataclysmic variable stars
Acesso em linha:	https://doi.org/10.3847/1538-4357/adc1b9
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