Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/6465
Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Rajamohan, R | - |
dc.date.accessioned | 2013-12-13T16:02:00Z | - |
dc.date.available | 2013-12-13T16:02:00Z | - |
dc.date.issued | 1973 | - |
dc.identifier.citation | Asundi, R.K., and Abhyankar, K.D eds. Proceedings of a Symposium on Spectroscopic Studies of Astrophysical Interest, 16 to 18 August 1972 | en |
dc.identifier.uri | http://hdl.handle.net/2248/6465 | - |
dc.description | Open Access | en |
dc.description.abstract | Rotational velocities and intensities of hydrogen and helium lines for over 40 members of the Scorpio Centaurus association are presented. From the measured equivalent width of Hr and Hd some evidence is found for the age difference between the upper Scorpius and upper Centaurus sub-groups. | en |
dc.language.iso | en | en |
dc.publisher | Centre of Advanced Study in Astronomy,Osmania University | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1973ssai.conf..121R | en |
dc.rights | © Centre of Advanced Study in Astronomy,Osmania University | en |
dc.title | Spectroscopy of Scorpi-Centaurus association | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Spectroscopy of Scorpi-Centaurs Association.pdf | Open Access | 126.14 kB | Adobe PDF | View/Open |
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