Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3313
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBombaci, I-
dc.contributor.authorThampan, A. V-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-09-01T10:35:52Z-
dc.date.available2008-09-01T10:35:52Z-
dc.date.issued2000-10-
dc.identifier.citationAstrophysical Journal, Vol. 541, No. 2, Part 2, pp. L71 - L74en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/3313-
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.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/312897en
dc.subjectEquation of Stateen
dc.subjectRelativityen
dc.subjectStars: Neutronen
dc.titleRapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matteren
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter67.33 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.