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Galactic plane structure in hard X-rays
Published online by Cambridge University Press: 21 October 2010
Abstract
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We study the structure of the Galaxy in the hard X-ray energy band (¿20 keV) using data from the INTEGRAL observatory. The increased sensitivity of the survey and the very deep observations performed during six years of the observatory operation allow us to detect about a hundred new sources. This significantly enlarges the sample of hard X-ray sources in the Galactic disk and bulge in a comparison with the previous studies.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 809
- Copyright
- Copyright © International Astronomical Union 2010
References
Lutovinov, A., Revnivtsev, M., Gilfanov, M., & Sunyaev, R., 2006, IAUS 230, 340 (Eds. Meurs, E.J.A., Fabbiano, G.; CUP)Google Scholar
Lutovinov, A., Revnivtsev, M., Gilfanov, M., & Sunyaev, R., 2008, Proceedings of the 6th INTEGRAL Workshop, 2007, ESA SP-622, p.241 (Eds. S.Grebenev, R.Sunyaev, C.Winkler)Google Scholar
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