dc.contributor.author |
Venkataraman, V |
|
dc.contributor.author |
Anandarao, B. G |
|
dc.date.accessioned |
2006-03-14T09:48:04Z |
|
dc.date.available |
2006-03-14T09:48:04Z |
|
dc.date.issued |
2005-06 |
|
dc.identifier.citation |
BASI, Vol. 33, No. 2, pp. 141-144 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/763 |
|
dc.description.abstract |
We report initial results from the near-infrared continuum studies on the massive star forming region IRAS 21413+5442. The colour-colour diagram and colour-magnitude diagram were used to determine the evolutionary stage and type of the central object powering the compact HII region. Distance to the object is estimated from H band flux in combination with published radio continuum fluxes |
en |
dc.format.extent |
247795 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 |
star formation |
en |
dc.subject |
compact HII region |
en |
dc.subject |
infrared photometry |
en |
dc.subject |
IRAS sources |
en |
dc.subject |
IRAS 21413+5442 |
en |
dc.title |
A near-infrared photometric study of the massive star forming region IRAS 21413+5442 |
en |
dc.type |
Article |
en |