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 |