Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/477
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Krishna Swamy, K. S | - |
dc.date.accessioned | 2005-08-09T04:56:08Z | - |
dc.date.available | 2005-08-09T04:56:08Z | - |
dc.date.issued | 1975-12 | - |
dc.identifier.citation | BASI, Vol. 3, No. 4, pp. 80 | en |
dc.identifier.uri | http://hdl.handle.net/2248/477 | - |
dc.format.extent | 204040 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | Astronomical Society of India | en |
dc.subject | Stars | en |
dc.title | Possible Detection of 33 mu Silicate feature in Cool Stars | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
KRISHNA SWAMY.pdf | 199.26 kB | Adobe PDF | View/Open |
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