Chandrasekhar, Subrahmanyan ; Ferrari, Valeria (1991) On the non-radial oscillations of a star III. A reconsideration of the axial modes Proceedings of the Royal Society of London Series A: Mathematical, Physical & Engineering Sciences, 434 (1891). pp. 449-457. ISSN 0962-8444
![[img]](http://repository.ias.ac.in/style/images/fileicons/application_pdf.png)
|
PDF
- Publisher Version
972kB |
Official URL: http://rspa.royalsocietypublishing.org/content/434...
Related URL: http://dx.doi.org/10.1098/rspa.1991.0104
Abstract
It is shown that for stars with radii in the range 2.25 GM/c2< R < ca. 3GM/c2, quasinormal axial modes of oscillation are possible. These modes are explicitly evaluated for stellar models of uniform energy density.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Royal Society Publishing. |
| ID Code: | 21125 |
| Deposited On: | 20 Nov 2010 09:06 |
| Last Modified: | 17 May 2016 05:20 |
Repository Staff Only: item control page
