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2014MNRAS.440.3275S - Mon. Not. R. Astron. Soc., 440, 3275-3284 (2014/June-1)
Broad iron emission line and kilohertz quasi-periodic oscillations in the neutron star system 4U 1636-53.
SANNA A., MENDEZ M., ALTAMIRANO D., BELLONI T., HIEMSTRA B. and LINARES M.
Abstract (from CDS):
Our results suggest that either the kHz QPO or the standard relativistic Fe line interpretation does not apply for this system. Furthermore, the simultaneous detection of kHz QPOs and broad iron lines is difficult to reconcile with models in which the broadening of the iron line is due to the reprocessing of photons in an outflowing wind.
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): accretion, accretion discs - stars: individual: 4U 1636-53 - stars: neutron - X-rays: binaries
Simbad objects: 5
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