activity
19962014
most citedCobalt-56 gamma-ray emission lines from the type Ia supernova 2014J

176 citations · 222 across the 3 of their papers we have counts for

collaborators

19 papers

astro-ph.HE2014★ 176 cited

Cobalt-56 gamma-ray emission lines from the type Ia supernova 2014J

E. Churazov, R. Sunyaev, J. Isern +8

A type Ia supernova is thought to be a thermonuclear explosion of either a single carbon-oxygen white dwarf or of a pair of merging white dwarfs. The explosion fuses a large amount…

astro-ph.CO2014★ 3 cited

Scattering of emission lines in galaxy cluster cores: measuring electron temperature

S. Khedekar, E. Churazov, S. Sazonov +2

The central galaxies of some clusters can be strong emitters in the Ly and H lines. This emission may arise either from the cool/warm gas located in the cool core of the clus…

astro-ph.HE2013★ 43 cited

Resonant scattering in the Perseus Cluster: spectral model for constraining gas motions with Astro-H

I. Zhuravleva, E. Churazov, R. Sunyaev +6

X-ray spectra from cores of galaxy clusters can be strongly distorted by resonant scattering of line photons, affecting metal abundance and gas velocity measurements. We introduce…

astro-ph.HE2012

Contribution of the accretion disk, hot corona, and obscuring torus to the luminosity of Seyfert galaxies: INTEGRAL and Spitzer observations

S. Sazonov, S. P. Willner, A. D. Goulding +12

We estimate the relative contributions of the supermassive black hole (SMBH) accretion disk, corona, and obscuring torus to the bolometric luminosity of Seyfert galaxies, using Spi…

astro-ph.HE2011

Resonant scattering in galaxy clusters for anisotropic gas motions on various spatial scales

I. Zhuravleva, E. Churazov, S. Sazonov +2

The determination of characteristic amplitudes and anisotropy of hot gas motions in galaxy clusters from observations of the brightest resonance lines is discussed. Gas motions aff…

astro-ph.GA2011

Luminosity function of faint Galactic sources in the Chandra bulge field

M. Revnivtsev, S. Sazonov, W. Forman +2

We study the statistical properties of faint X-ray sources detected in the Chandra Bulge Field. The unprecedented sensitivity of the Chandra observations allows us to probe the pop…