Chandra Observations of the Well-Studied 180 Myr Old Open Cluster M35

Details Chandra Observations of the Well-Studied 180 Myr Old Open Cluster M35 Chandra Observations of the Well-Studied 180 Myr Old Open Cluster M35

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21813303m&link_type=abstract

American Astronomical Society, AAS Meeting #218, #133.03; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

M35 is a relatively close ( 800 pc), rich, young ( 180 Myr) open cluster which has been the focus of extensive multi-epoch spectroscopic and photometric study. Some 250 single and 100 binary stars ( 50 with orbits) are confirmed members and 310 have measured rotation periods. This detailed information about membership, binarity, and rotation, makes M35 an ideal target for studying not only the rotation-activity-age relation for cool stars, but also for the effect of a stellar companion on this relationship. We present preliminary results of a 130 ksec ACIS-I observation near the core of the M35, containing 180 cluster members. We explore how the coronal flux and temperature change across the cluster's color-period diagram, how binarity affects these results, and compare our findings with other clusters.
This work was funded by Chandra Award No. GO0-11041A.

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