========================================================================== J/A+A/473/149 Photometry of sources in IRAS 16362-4845 cluster (Comeron+, 2007) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table2.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/473/149 ==========================================================================
drwxr-xr-x 14 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 469 Jan 22 2008 .message -r--r--r-- 1 cats archive 3602 Jan 22 2008 ReadMe -rw-r--r-- 1 cats archive 1013 Jan 22 2008 +footg5.gif -rw-r--r-- 1 cats archive 2932 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 14301 Nov 18 2007 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/473/149 Photometry of sources in IRAS 16362-4845 cluster (Comeron+, 2007) ================================================================================ A close look at the heart of RCW 108. Comeron F., Schneider N. <Astron. Astrophys., 473, 149-162 (2007)> =2007A&A...473..149C ================================================================================ ADC_Keywords: Clusters, open ; Infrared sources ; Photometry, infrared Keywords: ISM: HII regions - ISM: individual objects: RCW 108 - stars: luminosity function, mass function - open clusters and associations: IRAS 16362-4845 Abstract: The IRAS 16362-4845 star-forming site in the RCW 108 complex contains an embedded compact cluster that includes some massive O-type stars. Star formation in the complex, and in particular in IRAS 16362-4845, has been proposed to be externally triggered by the action of NGC 6193. We present a photometric study of the IRAS 16362-4845 cluster sensitive enough to probe the massive brown dwarf regime. In particular, we try to verify an apparent scarcity of solar-type and low-mass stars reported in a previous paper (Comeron et al., 2005A&A...433..955C). Description: Our observations were carried out in service mode using NACO, the adaptive optics near-infrared camera and spectrograph at the VLT, in imaging mode. The observations were obtained on six different nights between 29/30 June and 28/29 July 2006.
© UDS/CNRS