Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.356..801f&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 356, Issue 3, pp. 801-809.
Astronomy and Astrophysics
Astronomy
5
Hii Regions, Ism: Individual: G333.6-0.2, Infrared: Ism
Scientific paper
We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6-0.2. The slope of the K-luminosity function towards the region (0.24 +/- 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H-K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the HII region.
Aitken David K.
Fujiyoshi Takuya
Lumsden Stuart L.
Moore Toby J. T.
Roche Patrick F.
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