dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Nandy, K |
|
dc.date.accessioned |
2008-09-24T14:48:47Z |
|
dc.date.available |
2008-09-24T14:48:47Z |
|
dc.date.issued |
1986-09 |
|
dc.identifier.citation |
Monthly Notices of Royal Astronomical Society, Vol. 222, No. 2, pp. 357 - 364 |
en |
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3885 |
|
dc.description.abstract |
The IRAS observations of R Cr B, SU Tau and V 348 Sgr indicate the existence of a cool dust component of temperature about 30 K in R Cr B and SU Tau and less than or equal to 100 K in V 348 Sgr, in addition to the hot dust. It is suggested that this cool dust shell is a remnant of the stage when these stars were red giants for the first time. Although R Cr B was observed by IRAS during a visual light minimum no significant IR flux increase was apparent. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Royal Astronomical Society |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1986MNRAS.222..357K |
en |
dc.subject |
Infrared astronomy satellite |
en |
dc.subject |
Spaceborne astronomy |
en |
dc.subject |
Stellar evolution |
en |
dc.subject |
Stellar spectrophotometry |
en |
dc.subject |
Stellar temperature |
en |
dc.subject |
Variable stars |
en |
dc.subject |
Cosmic dust |
en |
dc.subject |
Red giant stars |
en |
dc.subject |
Stellar envelopes |
en |
dc.title |
IRAS observations of R Cor Bor stars |
en |
dc.type |
Article |
en |