Stellar population in Chamaeleon I (Luhman, 2007)

Details Stellar population in Chamaeleon I (Luhman, 2007) Stellar population in Chamaeleon I (Luhman, 2007)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..21730104l&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/173/104. Originally published in: 2007ApJS..173..104L

Physics

Effective Temperatures, Photometry: Ri, Extinction, Photometry: Infrared, Stars: Pre-Main Sequence, Ysos

Scientific paper

Optical and near-IR broadband photometry from several sources (2MASS and DENIS for IK1 & IK2) were used to perform four surveys (IK1, RI, IK2, IZ). For RI, on the night of 2004 January 11, R- and I-band images obtained with the Inamori Magellan Areal Camera and Spectrograph (IMACS) on the Magellan I telescope at Las Campanas Observatory were used. Deep optical and near-IR images of the densest portion of the southern subcluster that were obtained by Luhman et al. (2005ApJ...635L..93L,) collected with the Advanced Camera for Surveys (ACS) aboard HST through the F775W and F850LP filters were used for IZ.
(6 data files).

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