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http://hdl.handle.net/2248/4718
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DC Field | Value | Language |
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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 |
Appears in Collections: | BASI Publications IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Interstellar dust studies with TAUVEX | 481.47 kB | Adobe PDF | View/Open |
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