Young Stellar Objects in the Large Magellanic Cloud Star-Forming Region N206

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

N206 (Henize 206) is an active star-forming region ( 93.5 kpc2) located at the southern edge of the Large Magellanic Cloud, southeast of the well-known 30 Doradus complex. New Spitzer IRAC mid-infrared mosaic photometry provided as part of the Surveying the Agents of a Galaxy's Evolution (SAGE) project in combination with optical data from the Magellanic Cloud Photometric Survey (MCPS), near-infrared data from the 2-Micron All-Sky-Survey (2MASS) and the Infrared Survey Facility (IRSF), and far-infrared SAGE data from the Spitzer MIPS 24 micron band has allowed us to discover a previously unseen population of Young Stellar Objects (YSOs). Through the use of Spectral Energy Distribution (SED) analysis (Robitaille et al), which fits our data points to a grid of 200,000 model SEDs, we were able to classify 178 objects as well-characterized YSO candidates. This is a factor of 25 more than the 7 which were previously identified as probable YSOs by Whitney et al (2008).

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

Young Stellar Objects in the Large Magellanic Cloud Star-Forming Region N206 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 Young Stellar Objects in the Large Magellanic Cloud Star-Forming Region N206, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Young Stellar Objects in the Large Magellanic Cloud Star-Forming Region N206 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1701902

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