Is the 6-ms binary pulsar the remnant of a bright galactic X-ray source?-Reference-Cited by-同舟云学术

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Is the 6-ms binary pulsar the remnant of a bright galactic X-ray source?

Published:1983-08 Issue:5925 Volume:304 Page:422-423
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Savonije G. J.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/304422a0.pdf

Reference13 articles.

1. Boriakoff, V., Buccheri, R. & Fanci, F. IAU Circ. No. 3806 (1983).

2. Webbink, R. F., Rappaport, S. & Savonije, G.J. Astrophys. J. (in the press).

3. Zahn, J. P. Astr. Astrophys. 57, 383–394 (1977).

4. Refsdal, S. & Weigert, A. Astr. Astrophys. 6, 426–440 (1970).

5. Refsdal, S. & Weigert, A. Astr. Astrophys. 13, 367–373 (1971).

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