dc.contributor.author |
Balachandra Kumar, K |
|
dc.contributor.author |
Raja, V |
|
dc.contributor.author |
Nagarajan, K |
|
dc.contributor.author |
Bagare, S. P |
|
dc.contributor.author |
Rajamanickam, N |
|
dc.date.accessioned |
2012-01-27T13:41:13Z |
|
dc.date.available |
2012-01-27T13:41:13Z |
|
dc.date.issued |
2002 |
|
dc.identifier.citation |
Baltic Astronomy, Vol. 11, pp. 529-535 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/5678 |
|
dc.description.abstract |
The transition probability parameters, Franck-Condon factors and r-centroids have been evaluated by a new more reliable numerical integration procedure for the bands of the PO molecule in the ultraviolet region (1800--2900 Å). These molecules are likely to be present in the atmospheres of cool stars and comets. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Institute of Theoretical Physics and Astronomy of Vilnius University |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2002BaltA..11..529B |
en |
dc.rights |
© Institute of Theoretical Physics and Astronomy |
en |
dc.subject |
Molecular data |
en |
dc.subject |
Frank-Condon factors |
en |
dc.subject |
PO molecule |
en |
dc.subject |
stars: late-type |
en |
dc.title |
Transition Probability Parameters for Certain Band Systems of the Astrophysical Molecule PO |
en |
dc.type |
Article |
en |