dc.contributor.author |
Srinivasan, G |
|
dc.date.accessioned |
2008-07-15T08:02:25Z |
|
dc.date.available |
2008-07-15T08:02:25Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 523 - 547 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2683 |
|
dc.description.abstract |
The choice of a suitable topic for this talk posed a problem for me. Should I talk about
some work I have done recently? Or, should I talk about something which is not yet
resolved, but of great contemporary Significance? The latter has the advantage that it
might inspire some of the younger persons in the audience to think about it. And that is
what I am going to do.
The topic I have chosen is the "Maximum Mass of Neutron Stars". This may appear
at first sight to be an academic question, an esoteric one at that (I); but this is not so. |
en |
dc.format.extent |
958522 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Neutron Stars |
en |
dc.subject |
Black Holes |
en |
dc.subject |
Mass Spectrum |
en |
dc.subject |
Nuclear Equilibrium |
en |
dc.title |
The maximum mass of neutron stars |
en |
dc.type |
Article |
en |