Spitzer-MIPS Observations of the eta Cha Young Association

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

To appear in The Astrophysical Journal

Scientific paper

10.1086/589708

We have mapped the eta Chamaeleontis young stellar association in the far-infrared with the Multiband Imaging Photometer for Spitzer (MIPS) on the Spitzer Space Telescope. All sixteen members within the map region were detected at 24 um, along with five members at 70 um and two at 160 um. Ten stars show far-infrared excess emission indicating the presence of circumstellar disks; six of these have central clearings as evidenced by the onset of excess emission at >5 um. No new infrared excess sources are identified among the 113 2MASS field stars with 24 um photometry but not seen as X-ray sources, indicating that membership lists derived from X-ray surveys are reasonably complete. Circumstellar disks in the eta Cha association span the range from 1e-1 to 1e-4 in their fractional infrared luminosity, with a median Ldust /Lstar of 0.04. The presence of optically thick, optically thin, and intermediate optical depth disks within the same stellar group, in combination with the large fraction of disks with inner holes, indicates that the Cha association represents a crucial stage in circumstellar disk evolution.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spitzer-MIPS Observations of the eta Cha Young Association does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spitzer-MIPS Observations of the eta Cha Young Association, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spitzer-MIPS Observations of the eta Cha Young Association will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-651425

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.