Other
Scientific paper
Jul 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sfet.confe..11v&link_type=abstract
"Star Formation in the Era of Three Great Observatories, meeting abstracts from the conference held July 13-15, 2005 in Cambridg
Other
Scientific paper
As part a programme of high resolution radio mapping of Galactic star forming regions, many Galactic star forming regions have been observed at 1280, 610 and 325 MHz using Giant Metrewave Radio Telescope (GMRT), India. GMRT is a synthesis telescope consisting of thirty 45 m diameter parabolic dishes spread in a 'Y' shape configuration. Baselines range from 100 m to 25 km providing high angular resolution (about 3" at 1280 MHz, 6" at 610 MHz and 9" at 325 MHz) as well as sensitivity to diffuse structures. In this paper some of the maps of southern sources will be presented. All the sources are resolved and many show extended diffuse emission. These maps will be compared with available maps at other wavelengths (e.g. millimeter, infrared) to have an understanding of these regions. Radiation transfer modeling of the observed spectral energy distribution from dust continuum, constrained by the radio emission and angular sizes will be presented.
Ghosh Sanjay K.
Kulkarni Vasant K.
Ojha Devendra K.
Tej Anandamayee
Verma Ram Prakash
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