Search Publications

Extragalactic X-ray discrete sources
DOI: 10.18372/2411-6602.16.01 Bibcode: 2020AstSR..16....1Z

Zadorozhna L. V.; Tugay A. V.; Shevchenko S. Yu.

Extra-galactic X-ray research with the launch of XMM-Newton has become the forefront of X-ray astronomy. X-ray sources outside our galaxy are the other galaxies - normal galaxies, radio galaxies, quasars, blazars, Seyfert galaxies, as well as extended sources in galaxy clusters - the glow of cluster's halo. X-ray space observatory's equipment reac…

2020 Astronomical School's Report
XMM-Newton 3
Observations of interacting galaxies NGC 2341 and NGC 2342 in X-ray band
DOI: 10.18372/2411-6602.14.12 Bibcode: 2018AstSR..14...81T

Tugay, A. V.; Shevchenko, S. Yu.; Ponomarenko, O. O.

The study of radiation of the interacting galaxies in different ranges enables to identify various processes occurring in them. The most active processes (such as star birth, material accretion onto the black holes, burster flashes, etc.) cause the appearance of X-rays. In our work, we studied the nature of the interacting pair of galaxies NGC 234…

2018 Astronomical School's Report
XMM-Newton 0
Approach of spacecraft Rosetta with comet 67P/Churyumov-Gerasimenko nucleus - the first scientific results
Bibcode: 2014AstSR..10...31C

Churyumov, K. I.

The first results of the study of the nucleus of comet Churyumov-Gerasimenko by Rosetta spacecraft are presented.

2014 Astronomical School's Report
Rosetta 1
Spectra of X-ray galaxies in filaments
DOI: 10.18372/2411-6602.09.1064 Bibcode: 2013AstSR...9...64T

Tugay, A. V.

Large-scale structure of Universe consists of galaxy clusters connected by filaments. Single filaments can be detected at redshifts up to 0.15. The general characteriscis of X-ray spectra of Sloan Digital Sky Survey galaxies, that lies outside clusters, are considered in this work. Seyfert 1 AGN's are the main type of X-ray sources in the selected…

2013 Astronomical School's Report
XMM-Newton 2
Features of the X-ray spectra of active galactic nuclei Mrk 1498
DOI: 10.18372/2411-6602.09.1080 Bibcode: 2013AstSR...9...80V

Vasylenko, A. A.; Fedorova, E. V.; Zhdanov, V. I.

We present results of our analysis of the XMM-Newton and Swift observations of the galaxy with Sy 1.9 active nucleus Mrk 1498. We analyze the spectra obtained from three EPIC cameras (PN and both MOS) within the 0.2-12 keV energy range and Swift/BAT instrument within the range of 14-195 keV. We demonstrate that for the X-ray spectrum of the AGN in…

2013 Astronomical School's Report
XMM-Newton 0
Solar stellar and substellar environment. I. Location in the galaxy and catalogues
DOI: 10.18372/2411-6602.08.1013 Bibcode: 2012AstSR...8...13Z

Zakhozhay, V. A.; Babenko, M. O.

Structure of the solar neighborhoods (ten parsecs space, Local stellar system and the Gould Belt), their place in the Galaxy and the distance from its center are analyzed. For the region within 10 pc from the Sun, except the stellar component, the contents of extrasolar planets and protoplanetary disks are presented. The catalogues of closest to S…

2012 Astronomical School's Report
Hipparcos 1
Space missions to the nuclei of comets - the key to understanding the cosmogony of the Solar system
DOI: 10.18372/2411-6602.08.1038 Bibcode: 2012AstSR...8...38C

Churyumov, K. I.

Some results obtained by space missions to the nuclei of some periodic comets, namely the mission "Ice", "Vega-1" and "Vega-2", "Suisei", "Sakigake", "Giotto", "Deep Space", "Stardust", "Deep Impact", "Epoxy", "Next" and the program and the scientific results of the mission "Rosetta" in the eight years of its flight to the nucleus of the comet 67P…

2012 Astronomical School's Report
Rosetta 0
X-Ray spectra of AGN's with strong emission lines
DOI: 10.18372/2411-6602.08.2160 Bibcode: 2012AstSR...8..160T

Tugay, A. V.; Vasylenko, A. A.; Zaetc, T. A.

Using XMM-Newton archive we obtained X-ray spectra for 12 AGN's with strong optical emission lines. Models of our spectra corresponds to Seyfert galaxies. We conclude that for Seyfert galaxies power-law spectral index in 2-12 keV band is less than 1.9 and minimal X-ray flux exceeds 1% of optical flux in u-band.

2012 Astronomical School's Report
XMM-Newton 0