dc.contributor.author |
Kilambi, G. C |
|
dc.contributor.author |
Nagar, P |
|
dc.contributor.author |
Kameswara Rao, N |
|
dc.date.accessioned |
2008-06-27T09:42:28Z |
|
dc.date.available |
2008-06-27T09:42:28Z |
|
dc.date.issued |
1992-06 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 13, No. 2, pp. 175 - 194 |
en |
dc.identifier.issn |
0250-6335 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/2524 |
|
dc.description.abstract |
Mid-ultraviolet and optical photometric analysis of helium stars are presented. A linear relation exists between the effective temperature derived from model atmospheres and (1965-V)0 index. The effective temperatures derived from (1965-V)0 index are somewhat higher than that of MK spectral type estimates especially for late B-type helium objects |
en |
dc.format.extent |
1339465 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1992JApA...13..175K |
en |
dc.subject |
ASTRONOMICAL PHOTOMETRY |
en |
dc.subject |
B STARS |
en |
dc.subject |
STELLAR ATMOSPHERES |
en |
dc.subject |
STELLAR SPECTRA |
en |
dc.subject |
STELLAR TEMPERATURE |
en |
dc.subject |
ULTRAVIOLET ASTRONOMY |
en |
dc.subject |
HELIUM |
en |
dc.subject |
RADIANT FLUX DENSITY |
en |
dc.subject |
ULTRAVIOLET SPECTRA |
en |
dc.title |
Mid-ultraviolet and optical photometry of helium stars |
en |
dc.type |
Article |
en |