An obscured cluster associated with RCW173 (Marco+, 2011)

Details An obscured cluster associated with RCW173 (Marco+, 2011) An obscured cluster associated with RCW173 (Marco+, 2011)

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35349114m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/534/A114. Originally published in: 2011A&A...534A.114M

Physics

Clusters: Open, Photometry: Ubv

Scientific paper

UBV photometry for roughly 600 stars in the vicinity of the HII region RCW 173 obtained with the Nordic Optical Telescope (La Palma) and reduced with IRAF version of DAOPHOT. The stars are distributed in three partially overlapping frames (A, B and C). Table 2 contains stars in frame A. Table 3 contains stars in frame B. Table 4 contains stars in frame C. Stars present in more than one frame are listed only once. We list X and Y positions with respect to each frame shown in Fig. 1 for all the stars in each frame, and their identification with objects in the 2MASS catalogue, together with their coordinates (right ascension (RA) and declination (DEC) in J2000). A few stars have no obvious corresponding source in the 2MASS catalogue. We identified these objects in the GLIMPSE catalogue (Benjamin et al., 2003PASP..115..953B) and assume their RA and DEC coordinates to be those assigned in this catalogue. A few stars have no counterparts in any of the two catalogues. The designation of each star is given by the letter that identifies the frame on which it is detected, plus a sequential number. Stars observed in more than one frame receive the designation corresponding to the frame with the highest number of measurements.
(3 data files).

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