A HARD X-RAY POWER-LAW SPECTRAL CUTOFF IN CENTAURUS X-4

A HARD X-RAY POWER-LAW SPECTRAL CUTOFF IN CENTAURUS X-4

The low-mass X-ray binary (LMXB) Cen X-4 is the brightest and closest (<1.2 kpc) quiescent neutron star transient. Previous 0.5-10 keV X-ray observations of Cen X-4 in quiescence identified two spectral components: soft thermal emission from the neutron star atmosphere and a hard power-law tail o...

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Bibliographic Details
Main Authors: Chakrabarty, Deepto, Tomsick, John A., Grefenstette, Brian W., Psaltis, Dimitrios, Bachetti, Matteo, Barret, Didier, Boggs, Steven E., Christensen, Finn E., Craig, William W., Furst, Felix, Hailey, Charles J., Harrison, Fiona A., Kaspi, Victoria, Miller, Jon M., Nowak, Michael A., Rana, Vikram, Stern, Daniel, Wik, Daniel R., Wilms, Jörn, Zhang, William W.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Institute of Physics/American Astronomical Society 2015
Online Access:http://hdl.handle.net/1721.1/95685
https://orcid.org/0000-0001-8804-8946

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http://hdl.handle.net/1721.1/95685
https://orcid.org/0000-0001-8804-8946

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