DSpace JSPUI
DSpace preserves and enables easy and open access to all types of digital content including text, images, moving images, mpegs and data sets
Learn More
Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/3640| Title: | Supernova SN 1987A - Rotation rate of the central pulsar |
| Authors: | Bhatt, H. C Datta, B |
| Keywords: | Pulsars Stellar Rotation Supernova 1987a Light Curve Stellar Luminosity Stellar Magnetic Fields Stellar Mass Accretion |
| Issue Date: | Apr-1989 |
| Publisher: | Royal Astronomical Society |
| Citation: | Monthly Notices of the Royal Astronomical Society, Vol. 237, pp. 1033 - 1036 |
| Abstract: | Using available observational data on supernova SN 1987A, firm quantitative lower limits on the rotation period of the central pulsar (assuming the pulsar luminosity to power the supernova light curve) are derived. It is also demonstrated that pulsars born in type II supernovae are, in general, unlikely to be fast pulsars. |
| URI: | http://hdl.handle.net/2248/3640 |
| ISSN: | 0035-8711 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Supernova SN 1987A - Rotation rate of the central pulsar | 399.54 kB | Adobe PDF |  View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.