X-ray Variability of the Milky Way

H.-J. Grimm; M. Gilfanov; R. Sunyaev

doi:10.1007/11403913_33

Growing Black Holes: Accretion in a Cosmological Context pp 181-182 | Cite as

X-ray Variability of the Milky Way

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Authors and affiliations

H.-J. Grimm
M. Gilfanov
R. Sunyaev

Observations of Supermassivbe Black Holes in Local Universe

First Online: 22 December 2005

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Part of the ESO Astrophysics Symposia book series (ESO)

Abstract

By constructing the power density spectrum of the Milky Way due to Galactic X-ray binaries (XRB) we investigate the prospect of disentangling the X-ray emission of galaxies due to SMBHs and X-ray binary populations for future X-ray missions.

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Authors and Affiliations

H.-J. Grimm
- 1
M. Gilfanov
- 2
R. Sunyaev
- 2

1.Harvard-Smithsonian Center for Astrophysics, Cambridge MA 02138USA
2.Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 GarchingGermany

About this paper

Cite this paper as:: Grimm HJ., Gilfanov M., Sunyaev R. () X-ray Variability of the Milky Way. In: Merloni A., Nayakshin S., Sunyaev R.A. (eds) Growing Black Holes: Accretion in a Cosmological Context. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg

DOI https://doi.org/10.1007/11403913_33
Publisher Name Springer, Berlin, Heidelberg
Print ISBN 978-3-540-25275-7
Online ISBN 978-3-540-31639-8
eBook Packages Physics and Astronomy

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