IIA Institutional Repository

Spectroscopy of Scorpio-Centaurus association

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account