dc.contributor.author |
Maheswar, G |
|
dc.contributor.author |
Muthu, C |
|
dc.contributor.author |
Sujatha, N. V |
|
dc.contributor.author |
Pandey, G |
|
dc.contributor.author |
Bhatt, H. C |
|
dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Murthy, J |
|
dc.date.accessioned |
2009-08-05T11:02:33Z |
|
dc.date.available |
2009-08-05T11:02:33Z |
|
dc.date.issued |
2007-06 |
|
dc.identifier.citation |
Bulletin of the Astronomical Society of India, Vol. 35, No. 2, pp. 233 - 238 |
en |
dc.identifier.issn |
0304-9523 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4718 |
|
dc.description.abstract |
We propose to carry out studies on the properties of inter- stellar dust using TAUVEX. Through the multi-band TAUVEX observations, particularly with the use of filters optimized for extinction observations of the 2175 ° feature, combined with optical observations and 2MASS archived data, A we can derive the extinction curve from UV to near-IR for stars located in dif- ferent regions and environments. The extinction curve is a sensitive indicator of the properties of the interstellar dust and, as such, will allow us to trace the properties and evolution of the interstellar dust as a function of environment. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://www.ncra.tifr.res.in/~basi/07June/Abstracts/352332007.htm |
en |
dc.rights |
© Astronomical Society of India |
en |
dc.subject |
ISM: Dust |
en |
dc.subject |
Extinction Galaxy: General |
en |
dc.title |
Interstellar dust studies with TAUVEX |
en |
dc.type |
Article |
en |