Relativistic Iron Line Emission from the Neutron Star Low-Mass X-Ray Binary 4U 1636-536

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, , Citation Dirk Pandel et al 2008 ApJ 688 1288 DOI 10.1086/592429

0004-637X/688/2/1288

Abstract

We present an analysis of XMM-Newton and RXTE data from three observations of the neutron star LMXB 4U 1636-536. The X-ray spectra show clear evidence of a broad, asymmetric iron emission line extending over the energy range 4-9 keV. The line profile is consistent with relativistically broadened Fe Kα emission from the inner accretion disk. The Fe Kα line in 4U 1636-536 is considerably broader than the asymmetric iron lines recently found in other neutron star LMXBs, which indicates a high disk inclination. We find evidence that the broad iron line feature is a combination of several Kα lines from iron in different ionization states.

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10.1086/592429