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• W2071409562 abstract "We present an accurate X-ray position of the massive globular cluster G1 obtained using XMM-Newton and the Hubble Space Telescope (HST). The X-ray emission of G1 has been detected recently with XMM-Newton. There are two possibilities for the origin of the X-ray emission: it could be due to either accretion of the central intermediate-mass black hole, or ordinary low-mass X-ray binaries. The precise location of the X-ray emission might distinguish between these two scenarios. By refining the astrometry of the XMM-Newton and HST data, we reduced the XMM-Newton error circle to 1.5''. Despite the smaller error circle, the precision is not sufficient to distinguish an intermediate-mass black hole or luminous low-mass X-ray binaries. This result, however, suggests that future Chandra observations may reveal the origin of the X-ray emission." @default.
• W2071409562 created "2016-06-24" @default.
• W2071409562 creator A5002708493 @default.
• W2071409562 date "2007-06-01" @default.
• W2071409562 modified "2023-09-23" @default.
• W2071409562 title "X‐Ray Localization of the Globular Cluster G1 withXMM‐Newton" @default.
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• W2071409562 doi "https://doi.org/10.1086/517880" @default.
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