Members of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?

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dc.creatorBagchi, Manjari
dc.creatorDey, Jishnu
dc.creatorKonar, Sushan
dc.creatorBhattacharya, Gour
dc.creatorDey, Mira
dc.date2006-10-15
dc.date2008-04-29
dc.date.accessioned2026-07-07T12:48:46Z
dc.date.available2026-07-07T12:48:46Z
dc.descriptionOne interesting method of constraining the dense matter Equations of State is to measure the advancement of the periastron of the orbit of a binary radio pulsar (when it belongs to a double neutron star system). There is a great deal of interest on applicability of this procedure to the double pulsar system PSR J0737-3039 (A/B). Although the above method can be applied to PSR A in future within some limitations, for PSR B this method can not be applied. On the other hand, the study of genesis of PSR B might be useful in this connection and its low mass might be an indication that it could be a strange star.
dc.description6 pages, no figure. Accepted for publication in New Astronomy
dc.identifierhttps://arxiv.org/abs/astro-ph/0610448
dc.identifierhttp://arxiv.org/abs/astro-ph/0610448
dc.identifierNew Astron.14:37,2009
dc.identifierdoi:10.1016/j.newast.2008.04.006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/222171
dc.subjectAstrophysics
dc.titleMembers of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?
dc.typetext

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