Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2518
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dc.contributor.authorSrinivasan, G.-
dc.date.accessioned2007-05-29T06:09:38Z-
dc.date.available2007-05-29T06:09:38Z-
dc.date.issued2001-
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.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.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
Appears in Collections:Research Papers (A&A)

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