dc.contributor.author |
Kochhar, R. K |
|
dc.date.accessioned |
2008-12-18T14:21:36Z |
|
dc.date.available |
2008-12-18T14:21:36Z |
|
dc.date.issued |
1981-03 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 2, pp. 87 - 93 |
en |
dc.identifier.issn |
0250-6335 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4115 |
|
dc.description.abstract |
We propose that single stars in the mass range 4–6·5M ⊙, that explode as Supernovae of Type I, are totally disrupted by the explosion and form shell-type remnants. More massive single stars which explode as Supernovae of Type II also give rise to shell-type remnants, but in this case a neutron star or a black hole is left behind. The first supernova explosion in a close binary also gives rise to a shell-type supernova remnant. The Crab-like filled-centre supernova remnants are formed by the second supernova explosion in a close binary. The hybrid supernova remnants, consisting of a filled centre surrounded by a shell, are formed if there is an active neutron star inside the shell. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1981JApA....2...87K |
en |
dc.relation.uri |
http://dx.doi.org/10.1007/BF02714245 |
en |
dc.subject |
Pulsars |
en |
dc.subject |
Supernovae |
en |
dc.subject |
Supernova remnants |
en |
dc.title |
On the relationship between pulsars and supernova remnants |
en |
dc.type |
Article |
en |