CONSTRAINTS ON THE NEUTRON STAR AND INNER ACCRETION FLOW IN SERPENS X-1 USING

CONSTRAINTS ON THE NEUTRON STAR AND INNER ACCRETION FLOW IN SERPENS X-1 USING

We report on an observation of the neutron star low-mass X-ray binary Serpens X-1, made with NuSTAR. The extraordinary sensitivity afforded by NuSTAR facilitated the detection of a clear, robust, relativistic Fe K emission line from the inner disk. A relativistic profile is required over a single Ga...

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Bibliographic Details
Main Authors: Miller, J. M., Parker, M. L., Fuerst, F., Bachetti, Matteo, Barret, Didier, Grefenstette, Brian W., Tendulkar, S., Harrison, Fiona A., Boggs, Steven E., Chakrabarty, Deepto, Christensen, Finn E., Craig, William W., Fabian, Andrew C., Hailey, Charles J., Natalucci, Lorenzo, Paerels, F. B. S., Rana, V., Stern, D. K., Tomsick, J. A., Zhang, W. W.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Astronomical Society 2014
Online Access:http://hdl.handle.net/1721.1/88267
https://orcid.org/0000-0001-8804-8946

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http://hdl.handle.net/1721.1/88267
https://orcid.org/0000-0001-8804-8946

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