Near-Infrared Photometric Variability of Stars toward the Chamaeleon I Molecular Cloud
Near-Infrared Photometric Variability of Stars toward the Chamaeleon I Molecular Cloud
We present the results of a J, H, and Ks photometric monitoring campaign of a 072 × 6° area centered on the Chamaeleon I star-forming region. Data were obtained on 15 separate nights over a 4 month time interval using the Two Micron All Sky Survey south telescope. Out of …