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On the limiting mass of neutron stars

dc.contributor.authorSrinivasan, G
dc.date.accessioned2007-05-29T06:09:38Z
dc.date.available2007-05-29T06:09:38Z
dc.date.issued2001
dc.descriptionRestricted Access.en
dc.description.abstractThe maximum mass of neutron stars is one of the most important predictions of the general relativistic theory of stellar structure. This paper highlights the difficulties in making a definitive prediction, and also reviews the progress made so far.en
dc.format.extent277808 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationBlack Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation: Proceedings of the ESO Workshop Held at Garching, Germany, 6-8 September 1999, in Honour of Riccardo Giacconi, ESO ASTROPHYSICS SYMPOSIA. Eds. L. Kaper, E.P.J. van den Heuvel, and P.A. Woudt. p45, Springer-Verlag, 2001.en
dc.identifier.isbn3-540-41581-5
dc.identifier.urihttp://hdl.handle.net/2289/2518
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2001bhbg.conf...45Sen
dc.relation.urihttp://dx.doi.org/10.1007/10720995_5en
dc.rights2001 Springer-Verlagen
dc.titleOn the limiting mass of neutron starsen
dc.typeArticleen

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