A GLIMPSE of Star Formation in the Giant H II Region RCW 49

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted by ApJS, Spitzer edition. 9 pages, 6 figures. Due to space limitations on astro-ph, figures 1-4 are submitted as sepa

Scientific paper

10.1086/422557

GLIMPSE imaging using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope indicates that star formation is ongoing in the RCW 49 giant H II region. A photometric comparison of the sources in RCW 49 to a similar area to its north finds that at least 300 stars brighter than 13th magnitude in band [3.6] have infrared excesses inconsistent with reddening due to foreground extinction. These are likely young stellar objects (YSOs) more massive than 2.5 M_sun suggesting that thousands more low-mass stars are forming in this cloud. Some of the YSOs are massive (B stars) and therefore very young, suggesting that a new generation of star formation is occurring, possibly triggered by stellar winds and shocks generated by the older (2-3 Myr) central massive cluster. The Spitzer IRAC camera has proven to be ideally suited for distinguishing young stars from field stars, and the GLIMPSE survey of the Galactic Plane will likely find thousands of new star formation regions.

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

A GLIMPSE of Star Formation in the Giant H II Region RCW 49 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 A GLIMPSE of Star Formation in the Giant H II Region RCW 49, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A GLIMPSE of Star Formation in the Giant H II Region RCW 49 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-58906

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