Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/4484Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Srinivasan, G. | - |
| dc.date.accessioned | 2012-05-14T09:27:31Z | - |
| dc.date.available | 2012-05-14T09:27:31Z | - |
| dc.date.issued | 1991 | - |
| dc.identifier.citation | Texas / Eso-Cern Symposium on Relativistic Astrophysics, Cosmology, and Fundamental Physics Vol647, p.538-547 | en |
| dc.identifier.issn | 0077-8923 | - |
| dc.identifier.uri | http://hdl.handle.net/2289/4484 | - |
| dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) | en |
| dc.language.iso | en | en |
| dc.publisher | Annals New York Academy Of Sciences | en |
| dc.rights | 1991 Annals New York Academy Of Sciences | en |
| dc.title | Evolution of the magnetic fields of neutron stars | en |
| dc.type | Article | en |
| Appears in Collections: | Research Papers (A&A) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 1991_Texas ESO-CERN Symposium on relativistic astrophysics cosmology and fundamental physics_p538.pdf Restricted Access | Restricted Access | 720.29 kB | Adobe PDF | View/Open Request a copy |
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