Advective Accretion onto a Nonspherical Accretor in White Dwarf and Neutron Star Binaries: A New Scenario of Shock Formation
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ac0e9e/pdf
Reference69 articles.
1. Slim accretion disks
2. Marginally stable orbits around Maclaurin spheroids and low-mass quark stars
3. Disk structure of cataclysmic variables and broadband noise characteristics in comparison with XRBs
4. Accretion flows in nonmagnetic white dwarf binaries as observed in X-rays
5. SWIFTX-RAY TELESCOPE OBSERVATIONS OF THE NOVA-LIKE CATACLYSMIC VARIABLES MV Lyr, BZ Cam, AND V592 Cas
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1. Two-temperature accretion flows around strongly magnetized stars and their spectral analysis;Monthly Notices of the Royal Astronomical Society;2023-04-13
2. 1RXH J082623.6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate;The Astrophysical Journal;2022-08-01
3. Characterizing the Advective Hot Flows of Nova-like Cataclysmic Variables in the X-Rays: The Case of BZ Cam and V592 Cas;The Astrophysical Journal;2022-06-01
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