Zobrazeno 1 - 10
of 143
pro vyhledávání: '"M., Revnivtsev"'
An unresolved X-ray glow (at energies above a few kiloelectronvolts) was discovered about 25 years ago and found to be coincident with the Galactic disk -the Galactic ridge X-ray emission. This emission has a spectrum characteristic of a 1e8 K optica
Externí odkaz:
http://arxiv.org/abs/0904.4649
Autor:
M. Pavlinsky, V. Akimov, V. Levin, A. Krivchenko, A. Rotin, M. Kuznetsova, I. Lapshov, A. Tkachenko, N. Semena, M. Buntov, A. Glushenko, V. Arefiev, A. Yaskovich, S. Grebenev, S. Sazonov, M. Revnivtsev, A. Lutovinov, S. Molkov, R. Krivonos, D. Serbinov, M. Kudelin, T. Drozdova, S. Voronkov, R. Sunyaev, E. Churazov, M. Gilfanov, V. Babyshkin, I. Lomakin, A. Menderov, M. Gubarev, B. Ramsey, K. Kilaru, S. L. O’Dell, J. Kolodziejczak, R. Elsner, V. Zavlin, D. Swartz
Publikováno v:
SPIE Proceedings.
Publikováno v:
Astrophysical Letters & Communications. Dec99 Pt 1, Vol. 38 Issue 1-6, p121. 4p. 1 Graph.
Autor:
M. Revnivtsev
Publikováno v:
Astronomy & Astrophysics. 410:865-870
We present an analysis of the Galactic bulge emission observed by the RXTE/PCA during a set of scans over the Galactic Center field, performed in 1999-2001. The total exposure time of these observations is close to 700 ksec. We construct the distribu
Autor:
R. A. Sunyaev, M. Revnivtsev
Publikováno v:
Astronomy Letters. 28:69-72
We present an upper limit on the 3--20 keV X-ray flux from the black hole - microlens OGLE-1999-BUL-32, based on RXTE/PCA scans over the Galactic Center region in 1999-2000. It is shown that the X-ray luminosity of the black hole did not exceed L(3-2
Autor:
M. Pavlinsky, V. Akimov, V. Levin, I. Lapshov, A. Tkachenko, N. Semena, V. Arefiev, A. Glushenko, A. Yaskovich, R. Burenin, S. Sazonov, M. Revnivtsev, M. Buntov, S. Grebenev, A. Lutovinov, M. Kudelin, S. Grigorovich, D. Litvin, V. Lazarchuk, I. Roiz, M. Garin, M. Gubarev, B. Ramsey, K. Kilaru, S. L. O'Dell, R. Elsner
Publikováno v:
SPIE Proceedings.
Autor:
V. Suleimanov, J. Poutanen, M. Revnivtsev, K. Werner, Ersin Göğüş, Ünal Ertan, Tomaso Belloni
Publikováno v:
SCOPUS0094243X-2011-1379-SID80053367573
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron stars in low mass X-ray binaries. Compton scattering is taken into account. The models were computed in LTE approximation for six different chemical compos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11b47c1db520e0066b4c8f1aeed637be
http://arxiv.org/abs/1010.0151
http://arxiv.org/abs/1010.0151
Autor:
Jonathan E. Grindlay, M. van den Berg, R. A. Burenin, D. I. Karasev, William R. Forman, M. Revnivtsev
We studied the stellar population in the central 6.6x6.6arcmin,region of the ultra-deep (1Msec) Chandra Galactic field - the "Chandra bulge field" (CBF) approximately 1.5 degrees away from the Galactic Center - using the Hubble Space Telescope ACS/WF
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4d25476b30671029b47f9ed6ea29111a
Autor:
M. Revnivtsev, V. Arefiev, Axel Schwope, V. Babyshkin, Andrea Santangelo, Hans Böhringer, J. H. M. M. Schmitt, S. Grigorovich, V. Levin, E. M. Churazov, Jörn Wilms, I. Lapshov, M. N. Pavlinsky, R. A. Sunyaev, M. Buntov, N. Semena, S. Sazonov, Günther Hasinger, Peter Predehl, Alexey Vikhlinin, V. Akimov
Publikováno v:
SPIE Proceedings.
The Spectrum-Roentgen-Gamma mission will be launched in the 2012 year into a L2 orbit with Soyuz launcher and Fregat buster from Baikonur. The mission will conduct all-sky survey with X-ray mirror telescopes eROSITA and ART-XC up to 11 keV. It will a
Autor:
Alexey Vikhlinin, Sergey Sazonov, William R. Forman, E. Churazov, M. Revnivtsev, R. A. Sunyaev
An unresolved X-ray glow (at energies above a few kiloelectronvolts) was discovered about 25 years ago and found to be coincident with the Galactic disk -the Galactic ridge X-ray emission. This emission has a spectrum characteristic of a 1e8 K optica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e272c5827b90cf094be06c26cd7516de
http://arxiv.org/abs/0904.4649
http://arxiv.org/abs/0904.4649