Spectroscopy of Scorpi-Centaurus association

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