dc.contributor.author |
Ghosh, S. K |
|
dc.date.accessioned |
2006-03-14T09:42:58Z |
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dc.date.available |
2006-03-14T09:42:58Z |
|
dc.date.issued |
2005-06 |
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dc.identifier.citation |
BASI, Vol. 33, No. 2, pp. 133-139 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/762 |
|
dc.description.abstract |
Studies of Galactic star forming regions being carried out at TIFR, is summarized. The techniques and typical results from these studies have been described brie y, which include: the balloon borne far infrared mapping in broad photometric bands (150 & 210mu m) as well as spectroscopic imaging in the fine structure [C II] line at 158 m; near infrared imaging in broad and narrow bands using the Mt. Abu Infrared Telescope & Himalayan Chandra Telescope; high resolution radio interferometric imaging in the 330-1400 MHz bands using GMRT; and use of data products from international space missions like Midcourse Space Experiment (MSX). |
en |
dc.format.extent |
388261 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
infrared |
en |
dc.subject |
ISM - stars |
en |
dc.subject |
formation - Galaxy |
en |
dc.title |
Star formation studies at TIFR |
en |
dc.type |
Article |
en |