Monitoring Chandra Observations of the Quasi-persistent Neutron Star X-Ray Transient MXB 1659-29 in Quiescence: The Cooling Curve of the Heated Neutron Star Crust-Reference-Cited by-同舟云学术

Monitoring Chandra Observations of the Quasi-persistent Neutron Star X-Ray Transient MXB 1659-29 in Quiescence: The Cooling Curve of the Heated Neutron Star Crust

Published:2004-04-07 Issue:1 Volume:606 Page:L61-L64
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Wijnands Rudy,Homan Jeroen,Miller Jon M.,Lewin Walter H. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference22 articles.

1. Arnaud, K. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & J. Barnes (San Francisco: ASP), 17

2. Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars

3. The neutron stars of Soft X-ray Transients

4. Aquila X-1 from Outburst to Quiescence: The Onset of the Propeller Effect and Signs of a Turned-on Rotation-powered Pulsar

5. Irregular X-ray variability in the transient X-ray burst source MXB 1659-29

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