MASS/RADIUS CONSTRAINTS ON THE QUIESCENT NEUTRON STAR IN M13 USING HYDROGEN AND HELIUM ATMOSPHERES-Reference-Cited by-同舟云学术

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MASS/RADIUS CONSTRAINTS ON THE QUIESCENT NEUTRON STAR IN M13 USING HYDROGEN AND HELIUM ATMOSPHERES

Published:2013-02-01 Issue:2 Volume:764 Page:145
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Catuneanu A.,Heinke C. O.,Sivakoff G. R.,Ho W. C. G.,Servillat M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/764/i=2/a=145/pdf

Reference57 articles.

1. The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter

2. Intermittent Millisecond X-Ray Pulsations from the Neutron Star X-Ray Transient SAX J1748.9-2021 in the Globular Cluster NGC 6440

3. DISCOVERY OF A 205.89 Hz ACCRETING MILLISECOND X-RAY PULSAR IN THE GLOBULAR CLUSTER NGC 6440

4. The relativistic pulsar-white dwarf binary PSR J1738+0333 - I. Mass determination and evolutionary history

5. Chandra X‐Ray ObservatoryObservations of the Globular Cluster M28 and Its Millisecond Pulsar PSR B1821−24

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