Near-Infrared Photometric Variability of Stars Toward the Chamaeleon I Molecular Cloud

Details Near-Infrared Photometric Variability of Stars Toward the Chamaeleon I Molecular Cloud Near-Infrared Photometric Variability of Stars Toward the Chamaeleon I Molecular Cloud

2002-04-25

arxiv.org/abs/astro-ph/0204430v1

Astronomy and Astrophysics

Astrophysics

To appear in AJ; see http://www.astro.caltech.edu/~jmc/variables/cham1/

Scientific paper

10.1086/341390

We present the results of a J, H, and K_s photometric monitoring campaign of a 0.72 x 6 sq deg. area centered on the Chamaeleon I star forming region. Data were obtained on 15 separate nights over a 4 month time interval using the 2MASS South telescope. Out of a total of 34,539 sources brighter than the photometric completeness limits (J=16.0, H=15.2, K_s=14.8), 95 exhibit near-infrared variability in one or more bands. The variables can be grouped into a population of bright, red objects that are associated with the Chamaeleon I association, and a population of faint, blue variables that are dispersed over the full 6 deg of the survey and are likely field stars or older pre-main-sequence stars unrelated to the present-day Chamaeleon I molecular cloud. Ten new candidate members of Chamaeleon I, including 8 brown dwarf candidates, have been identified based on variability and/or near-infrared excess emission in the J-H vs. H-K_s color-color-diagram. We also provide a compendium of astrometry and J, H, and K_s photometry for previously identified members and candidate members of Chamaeleon I.

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