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Interstellar dust studies with TAUVEX

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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


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