Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/956Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Nagar, P | - |
| dc.date.accessioned | 2006-04-13T04:30:10Z | - |
| dc.date.available | 2006-04-13T04:30:10Z | - |
| dc.date.issued | 1989-09 | - |
| dc.identifier.citation | BASI, Vol. 17, No. 3, pp. 60-69 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/956 | - |
| dc.description.abstract | A spectroscopic spot model has been developed incorporating spot magnetic fields. It is shown that the presence of spot magnetic field makes a noticeable effect on the shape of spectral lines | en |
| dc.format.extent | 820655 bytes | - |
| dc.format.mimetype | application/pdf | - |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of Indian | en |
| dc.subject | Stars | en |
| dc.subject | Starspots | en |
| dc.subject | Spot modelling | en |
| dc.title | Development of a stellar SPOT model | en |
| dc.type | Article | en |
| Appears in Collections: | BASI Publications | |
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