collaborators

9 papers

astro-ph.GA2026

Spectroscopic galaxy redshifts in the Peanut cluster -- a massive nearly head-on cluster merger shortly after pericenter passage

I. Zaznobin, N. Lyskova, I. Bikmaev +13

The Peanut cluster (SRGe J023820.8+200556, SRGe CL0238.3+2005, = 0.42) has recently emerged as a candidate for a rare, massive merger, potentially analogous to the Bulle…

astro-ph.SR2026

Study of Massive OBA Stars with X-ray Emission

E. A. Nikolaeva, I. F. Bikmaev, E. N. Irtuganov +3

A study of the physical parameters of a sample of 15 OBA-type stars with detected X-ray emission from the Spektr-RG/eROSITA telescope is presented. While X-ray emission from cool s…

astro-ph.HE2026

SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars

S. A. Prokhorenko, S. Yu. Sazonov, M. R. Gilfanov +5

Motivated by the idea of using quasars as standardizable candles for cosmology, we examine the relation between X-ray (at 2 keV, ) and ultraviolet (at 2500 Angstrom,…

astro-ph.HE2026

AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events

Yuhan Yao, Ryan Chornock, Andrew Mummery +39

We study AT2024kmq and AT2024lhc, two tidal disruption events (TDEs) with blue featureless spectra associated with high-mass black holes (). Both even…

astro-ph.HE2025

Identification of radio and gamma-ray pulsars in X-rays using data from the SRG/eROSITA all-sky survey

Yu. A. Shibanov, A. V. Karpova, D. A. Zyuzin +1

Using the data from the all-sky survey in soft X-rays performed by the eROSITA telescope onboard the Spectrum-Roentgen-Gamma observatory we identified known radio and -ray puls…

astro-ph.HE2025

Is the Fermi source 4FGL J1824.2+1231 a transitional millisecond pulsar?

D. A. Zyuzin, A. V. Karpova, A. Yu. Kirichenko +9

Transitional millisecond pulsars (tMSPs) in tight binary systems represent an important evolutionary link between low-mass X-ray binaries and radio millisecond pulsars. To date, on…