A near-infrared photometric study of the massive star forming region IRAS 21413+5442

Details A near-infrared photometric study of the massive star forming region IRAS 21413+5442 A near-infrared photometric study of the massive star forming region IRAS 21413+5442

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005basi...33..141v&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 33, Issue 2, p.141

Astronomy and Astrophysics

Astronomy

Star Formation, Compact Hii Region, Infrared Photometry, Iras Sources: Iras 21413+5442

Scientific paper

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.1

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