Comparison of Padova and Dartmouth Isochrones Using Deep Near Infrared Data for Key Open Clusters.

Details Comparison of Padova and Dartmouth Isochrones Using Deep Near Infrared Data for Key Open Clusters. Comparison of Padova and Dartmouth Isochrones Using Deep Near Infrared Data for Key Open Clusters.

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21915122t&link_type=abstract

American Astronomical Society, AAS Meeting #219, #151.22

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a comparison of results from using Padova and Dartmouth isochrones for several open clusters (M35, NGC 2158, M37, M67) in the infrared. Using newly reduced deep near infrared data (J 20), we compare the validity of these isochrones at low mass, and over a wide range in cluster ages. In addition, we combine the new deep NIR data with 2MASS, mid infrared photometry (3.0-8.0 micron) and optical (UBVRI) data to construct a wide photometric set for each cluster. We look for variations in isochrone-derived parameters when using different color-magnitude combinations.

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