Star Formation in the Cluster Enviroment of BD +40 4124

Details Star Formation in the Cluster Enviroment of BD +40 4124 Star Formation in the Cluster Enviroment of BD +40 4124

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.8507l&link_type=abstract

American Astronomical Society Meeting 205, #85.07; Bulletin of the American Astronomical Society, Vol. 36, p.1483

Astronomy and Astrophysics

Astronomy

Scientific paper

We present observations of the dense molecular gas associated with the Herbig Be star BD +40 4124. With the highest resolution imaging of the dense gas in the system to date, we detect several gas clumps that are associated with young stars and have estimated masses of around 1 solar mass. The strongest emission peak coincides with the position of the southern component of the binary V1318 Cyg, which suggests that this source is perhaps the youngest in the cluster. The compact dust emission, although closer to the southern component, is also extended in the direction of the northern source. Owing to the high spectral resolution, we confirm the suggestion that there is a gradient in linewidth along the north-south direction.

Affiliated with

Also associated with

No associations

Rating

Star Formation in the Cluster Enviroment of BD +40 4124 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 Star Formation in the Cluster Enviroment of BD +40 4124, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star Formation in the Cluster Enviroment of BD +40 4124 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1641533