I. Kotko
YOU?
Author Swipe
View article: The enigmatic origin of two dormant BH binaries: <i>Gaia</i> BH1 and <i>Gaia</i> BH2
The enigmatic origin of two dormant BH binaries: <i>Gaia</i> BH1 and <i>Gaia</i> BH2 Open
The two systems, namely, Gaia BH1 and Gaia BH2, that have been confirmed as dormant (i.e. no X-ray emission detected) black hole (BH) – low-mass star binaries in the latest Gaia mission data release are intriguing in the context of their f…
View article: The enigmatic origin of two dormant BH binaries: Gaia BH1 and Gaia BH2
The enigmatic origin of two dormant BH binaries: Gaia BH1 and Gaia BH2 Open
The two systems, namely, Gaia~BH1 and Gaia~BH2, that have been confirmed as dormant (i.e., no X-ray emission detected) black hole (BH) - low-mass star binaries in the latest Gaia mission data release (DR3) are intriguing in the context of …
View article: The X-ray binaries in M83: Will any of them form gravitational wave sources for LIGO-VIRGO-KAGRA?
The X-ray binaries in M83: Will any of them form gravitational wave sources for LIGO-VIRGO-KAGRA? Open
There are 214 X-ray point sources ( L X > 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 (NS) or a black hole (BH) from a companion or donor sta…
The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA? Open
There are 214 X-ray point-sources ($L_{\rm X}>10^{35} \mathrm{erg/s}$) identified as X-ray binaries (XRBs) in the nearby spiral galaxy M83. Since XRBs are powered by accretion onto a neutron star or a black hole from a companion/donor star…
Dwarf nova outbursts with magnetorotational turbulence Open
The phenomenological disc instability model has been successful in reproducing the observed light curves of dwarf nova outbursts by invoking an enhanced Shakura–Sunyaev α parameter ∼0.1–0.2 in outburst compared to a low value ∼0.01 in quie…