High-Resolution Near-IR Study of Regions of Massive Star Formation

Details High-Resolution Near-IR Study of Regions of Massive Star Formation High-Resolution Near-IR Study of Regions of Massive Star Formation

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..337a&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of high-resolution near-infrared (Js, H and Ks) imaging data obtained with the VLT/ISAAC instrument for IRAS 09002-4732 and IRAS 16177-5018, two luminous IR sources with radio continuum and molecular-line emission indicating ongoing massive star formation. The deep near-IR (NIR) images show two embedded clusters of young stars. We identify a population of pre-main sequence (PMS) stars according to their NIR excess.

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