dc.contributor.author |
Kamath, U. S |
|
dc.contributor.author |
Ashok, N. M |
|
dc.contributor.author |
Chandrasekhar, T |
|
dc.date.accessioned |
2007-09-27T11:14:41Z |
|
dc.date.available |
2007-09-27T11:14:41Z |
|
dc.date.issued |
1996 |
|
dc.identifier.citation |
BASI, Vol.24 No. 4 pp. 683-686 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/1837 |
|
dc.description.abstract |
JHK photometry of the slow, Fe-II type nova- Nova Aquilae 1995- obtained at the 1.2m Gurushikhar Infrared Telescope (GIRT) is presented here. Evidence for the presence of dust in the nova ejected based on these observations is discussed. |
en |
dc.format.extent |
179965 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1996BASI...24..683K |
en |
dc.subject |
Nova Aquliae |
en |
dc.subject |
infrared observations |
en |
dc.title |
Near-infrared observations of nova Aquilae 1995 |
en |
dc.type |
Article |
en |