Ultraluminous X-ray sources with He star companions
L Li, B Wang, D Liu, Y Guo, WC Chen… - Monthly Notices of the …, 2024 - academic.oup.com
Ultraluminous X-ray sources (ULXs) are non-nuclear point-like objects observed with
extremely high X-ray luminosity that exceeds the Eddington limit of a black hole. A fraction of …
extremely high X-ray luminosity that exceeds the Eddington limit of a black hole. A fraction of …
An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies
BD Lehmer, EB Monson, RT Eufrasio… - The Astrophysical …, 2024 - iopscience.iop.org
We present a new empirical framework modeling the metallicity and star formation history
(SFH) dependence of X-ray luminous (L≳ 10 36 erg s− 1) point-source population X-ray …
(SFH) dependence of X-ray luminous (L≳ 10 36 erg s− 1) point-source population X-ray …
Possible anticorrelations between pulsation amplitudes and the disc growth of Be stars in giant-outbursting Be X-ray binaries
M Niwano, MM Fausnaugh, RM Lau… - Monthly Notices of …, 2024 - academic.oup.com
The mechanism of X-ray outbursts in Be X-ray binaries remains a mystery, and
understanding their circumstellar discs is crucial for a solution of the mass-transfer problem …
understanding their circumstellar discs is crucial for a solution of the mass-transfer problem …
An alternative model for the orbital decay of M82 X-2: the anomalous magnetic braking of a Bp star
WC Chen - The Astrophysical Journal, 2024 - iopscience.iop.org
An Alternative Model for the Orbital Decay of M82 X-2: The Anomalous Magnetic Braking of a
Bp Star - IOPscience Skip to content IOP Science home Accessibility Help Search Search all …
Bp Star - IOPscience Skip to content IOP Science home Accessibility Help Search Search all …
The X-ray binaries in M83: Will any of them form gravitational wave sources for LIGO-VIRGO-KAGRA?
I Kotko, K Belczynski - Astronomy & Astrophysics, 2024 - aanda.org
There are 214 X-ray point sources (LX> 10 35 erg s− 1) identified as X-ray binaries (XRBs)
in the nearby spiral galaxy M83. Since XRBs are powered by accretion onto a neutron star …
in the nearby spiral galaxy M83. Since XRBs are powered by accretion onto a neutron star …