... With the exception of NGC5128 (the radio galaxy Centaurus A), for which the XLF has ... young or rejuvenated E and S0 galaxies resulting from recent mergers (e.g., NGC5128 ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2006_N3379_N4278_XLF.pdf -- 358.3 Кб -- 06.12.2010 Похожие документы
... LMXB populations of the nearby galaxies NGC5128 and M31 significantly flatten below ... 1 .It was also suggested, both in M31 and NGC5128, that the XLF of GC-LMXBs may be ...
... Additionally, we used the published results for GC-LMXBs in NGC 3379, 4278, and 4697 from Kim et al. (2009), and in Cen A (NGC5128) and the bulge of M31 from Voss et al. (2009) to supplement the number of very faint LMXBs (Section 5.2). ...
... Additionally, we used the published results for GC-LMXBs in NGC 3379, 4278 and 4697 from Kim et al. (2009), and in Cen A (NGC5128) and the bulge of M31 from Voss et al. (2009) to supplement the number of very faint LMXBs (section 5.2). ...
... For NGC5128 (Cen A), which is rather complex with jets and various features, we take LX,Gas (corrected for a different distance and energy band) from Kraft et al. (2003), who analyzed Chandra ACIS-I and XMM-Newton data. ...
... Sarazin et al. (2003) reported a weak tendency for bright LMXBs to avoid GCs and Minniti et al. (2004) reported that no bright GC LMXB (i.e., BH candidates) is identified in NGC5128. ...
... We present the results from a study of the X-ray point source population in two Chandra X-ray Observatory observations of the nearby radio galaxy Centaurus A (NGC5128). ...