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), equ...
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Published in | The Astrophysical journal Vol. 984; no. 1; pp. 9 - 21 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
The American Astronomical Society
01.05.2025
IOP Publishing |
Subjects | |
Online Access | Get full text |
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