Neutron star cooling and the rp process in thermonuclear X-ray bursts-Reference-Cited by-同舟云学术

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Neutron star cooling and the rp process in thermonuclear X-ray bursts

Published:2017-10 Issue: Volume:606 Page:A130
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

in ’t Zand J. J. M.,Visser M. E. B.,Galloway D. K.,Chenevez J.,Keek L.,Kuulkers E.,Sánchez-Fernández C.,Wörpel H.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201731281/pdf

Reference93 articles.

1. A broad spectral band Indian Astronomy satellite ‘Astrosat’

2. Arnaud, K. A. 1996, in Astronomical Data Analysis Software and Systems V, eds. G. H. Jacoby, & J. Barnes, ASP Conf. Ser., 101, 17

3. Indications for a slow rotator in the Rapid Burster from its thermonuclear bursting behaviour

4. Double-peaked thermonuclear bursts at the soft–hard state transition in the Rapid Burster

5. A RAY-TRACING ALGORITHM FOR SPINNING COMPACT OBJECT SPACETIMES WITH ARBITRARY QUADRUPOLE MOMENTS. II. NEUTRON STARS

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