dc.contributor.author | Babu, G. S. D. | |
dc.contributor.author | Sinvhal, S. D. | |
dc.date.accessioned | 2012-01-04T06:05:40Z | |
dc.date.available | 2012-01-04T06:05:40Z | |
dc.date.issued | 1972 | |
dc.identifier.uri | http://hdl.handle.net/123456789/894 | |
dc.description.abstract | A statistical study of magnetic stars reveals that their mean rotational velocities do not depend on their magnetic field strengths. Also that stars with low magnetic field strengths are mostly Mn stars and those with high field strengths are mostly Cr-Sr stars. | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartofseries | bac23-297 | |
dc.subject | Stars-Magnetic | en_US |
dc.title | On magnetic stars | en_US |
dc.type | Article | en_US |