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The Binary Pulsar PSR 1908+00 in NGC 6760

Deich, W. T. S. and Middleditch, J. and Anderson, S. B. and Kulkarni, S. R. and Prince, Thomas A. and Wolszczan, A. (1993) The Binary Pulsar PSR 1908+00 in NGC 6760. Astrophysical Journal Letters, 410 (2). L95-L98. ISSN 2041-8205. http://resolver.caltech.edu/CaltechAUTHORS:20141117-104837786

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Abstract

We present orbital parameters of the 3.6 ms binary pulsar 1908 +00 in the globular cluster NGC 6760. The orbital period is 3.4 hr, and the mass function is 3 x 10^6 M_⊙ , implying a minimum companion mass of 0.018 M_⊙ . The companion is probably degenerate; and if it is hydrogen, it is close to overflowing its Roche lobe. The only other millisecond binary radio pulsar systems with orbital period < 10 hr and mass function below 10-3 M_⊙ are the eclipsing pulsar 1957+20 and 1744-24A, and the very low mass binary 0021-721. These pulsars are ablating their companions and may be the progenitors of isolated millisecond pulsars. PSR 1908+00 shows no evidence for long-duration eclipses as are seen in 1744-24A, but short-duration eclipses as in 1957 + 20 are not excluded.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1993ApJ...410L..95DADSArticle
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Prince, Thomas A.0000-0002-8850-3627
Additional Information:© 1993. The American Astronomical Society.
Group:Space Radiation Laboratory
Non-Subject Keywords:binaries: general; pulsars: individual; stars: neutron
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1997-35
Record Number:CaltechAUTHORS:20141117-104837786
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20141117-104837786
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:51840
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:20 Nov 2014 04:48
Last Modified:27 Nov 2017 18:23

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