Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2
Fujiyoshi, T.; Smith, C.H.; Moore, T.J.T.; Lumsden, S.; Aitken, D.; Roche, P.F.
Citation: Fujiyoshi , T , Smith , C H , Moore , T J T , Lumsden , S , Aitken , D & Roche , P F 2005 , ' Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2 ' Monthly Notices of the Royal Astronomical Society , vol 356 , no. 3 , pp. 801-809 .
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 H ii region.
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2004.08501.x [Full text of this article is not available in the UHRA]