Zobrazeno 1 - 10
of 182
pro vyhledávání: '"Grimm, H J."'
Publikováno v:
Astrophys.J.690:128-142,2009
We present a system of X-ray photometry for the Chandra satellite. X-ray photometry can be a powerful tool to obtain flux estimates, hardness ratios, and colors unbiased by assumptions about spectral shape and independent of temporal and spatial chan
Externí odkaz:
http://arxiv.org/abs/0808.3718
We discuss the dynamics of microquasar jets in the interstellar medium, with specific focus on the effects of the X-ray binaries' space velocity with respect to the local Galactic standard of rest. We argue that, during late stages in the evolution o
Externí odkaz:
http://arxiv.org/abs/0808.1927
In this paper we investigate the X-ray spectra and X-ray spectral variability of compact X-ray sources for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and the star forming region NGC 604. In the
Externí odkaz:
http://arxiv.org/abs/0706.3927
Autor:
Heinz, S., Grimm, H. -J.
Publikováno v:
Astrophys.J.633:384-397,2005
By combining the recently derived X-ray luminosity function for Galactic X-ray binaries (XRBs) by Grimm et al. (2002) and the radio-X-ray-mass relation of accreting black holes found by Merloni et al. (2003), we derive predictions for the radio lumin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508277
In this paper we present the source list for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and on the star forming region NGC 604. We detect a total of 261 sources in an area of \~0.2 square degree
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506353
Publikováno v:
Mon.Not.Roy.Astron.Soc. 351 (2004) 1365
We study the statistical properties of the combined emission of a population of discrete sources (e.g. X-ray emission of a galaxy due to its X-ray binaries population). Namely, we consider the dependence of their total luminosity L_tot=SUM(L_k) and o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312540
Publikováno v:
Nucl.Phys.Proc.Suppl.132:369-375,2004
Based on recent X-ray observations of the Milky Way, Magellanic Clouds and nearby starburst galaxies we study population of high mass X-ray binaries, their connection with ultra-luminous X-ray sources and relation to the star formation. Although more
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309725
Publikováno v:
Mon.Not.Roy.Astron.Soc.347:L57,2004
We compare the results of Grimm et al. (2003) and Ranalli et al. (2003) on the Lx-SFR relation in normal galaxies. Based on the Lx-stellar mass dependence for LMXBs, we show, that low SFR (SFR<1 Msun/year) galaxies in the Ranalli et al. sample are co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301331
Publikováno v:
Mon.Not.Roy.Astron.Soc. 339 (2003) 793
Based on CHANDRA observations of nearby starburst galaxies and RXTE/ASM, ASCA and MIR-KVANT/TTM studies of high mass X-ray binary (HMXB) populations in the Milky Way and Magellanic Clouds, we propose that the number and/or the collective X-ray lumino
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205371
Publikováno v:
Astron.Astrophys.391:923-944,2002
We study the Log(N)-Log(S) and X-ray luminosity function in the 2-10 keV energy band, and the spatial (3-D) distribution of bright, log(L_X) > 34-35 erg/s, X-ray binaries in the Milky Way. In agreement with theoretical expectations and earlier result
Externí odkaz:
http://arxiv.org/abs/astro-ph/0109239