Spectroscopy of Scorpio-Centaurus association

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6403

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DC Field	Value	Language
dc.contributor.author	Rajamohan, R	-
dc.date.accessioned	2013-10-04T13:33:03Z	-
dc.date.available	2013-10-04T13:33:03Z	-
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, pp. 121-128	en
dc.identifier.uri	http://hdl.handle.net/2248/6403	-
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 H alpha and H delta 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.rights	© Centre of Advanced Study in Astronomy,Osmania University	en
dc.title	Spectroscopy of Scorpio-Centaurus association	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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