WFI optical photometry in Cha II dark cloud (Spezzi+, 2007)

Details WFI optical photometry in Cha II dark cloud (Spezzi+, 2007) WFI optical photometry in Cha II dark cloud (Spezzi+, 2007)

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34700281s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/470/281. Originally published in: 2007A&A...470..281S

Other

Molecular Clouds, Stars: Pre-Main Sequence, Photometry

Scientific paper

Table 7 reports the optical photometry of 73 objects in the Chamaeleon II (Cha II) dark cloud.
These data are part of an optical multi-band survey for low-mass pre-main sequence stars and young brown dwarfs in Cha II, performed using the wide-field imager (WFI) at the ESO 2.2m telescope.
As clarified in the last column, the table contains the confirmed members of Cha II, the candidates selected by previous surveys, and the new candidates selected in this work, as well as other sources identified as possible candidates in previous studies but that were rejected by our selection criteria.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

WFI optical photometry in Cha II dark cloud (Spezzi+, 2007) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with WFI optical photometry in Cha II dark cloud (Spezzi+, 2007), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WFI optical photometry in Cha II dark cloud (Spezzi+, 2007) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1721531