Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1485
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dc.contributor.authorBombaci, Ignazio-
dc.contributor.authorThampan, Arun V.-
dc.contributor.authorDatta, Bhaskar-
dc.date.accessioned2006-10-19T04:41:45Z-
dc.date.available2006-10-19T04:41:45Z-
dc.date.issued2000-10-01-
dc.identifier.citationThe Astrophysical Journal, 2000, Volume 541, Issue 2, pp. L71-L74en
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357(Online)-
dc.identifier.urihttp://hdl.handle.net/2289/1485-
dc.description.abstractFor a new equation of state of strange quark matter, we construct equilibrium sequences of rapidly rotating strange stars in general relativity. The sequences are the normal and supramassive evolutionary sequences of constant rest mass. We also calculate equilibrium sequences for a constant value of Ω corresponding to the most rapidly rotating pulsar PSR 1937+21. In addition, we calculate the radius of the marginally stable orbit and its dependence on Ω, relevant for modeling of kilohertz quasi-periodic oscillations in X-ray binaries.en
dc.format.extent68948 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe University of Chicago Press for the American Astronomical Societyen
dc.relation.urihttp://dx.doi.org/10.1086/312897en
dc.rights(2000) by the American Astronomical Society.en
dc.subjectEquation of State,en
dc.subjectRelativity,en
dc.subjectStars: Neutronen
dc.titleRapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matteren
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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