Outflows of Massive Stars in Cluster

Details Outflows of Massive Stars in Cluster Outflows of Massive Stars in Cluster

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998chphl..15..310m&link_type=abstract

Chinese Physics Letters, Volume 15, Issue 4, pp. 310-312 (1998).

Physics

Scientific paper

Massive stars often tend to be in cluster when they form in molecular clouds, and bipolar molecular outflows occur during the forming process of stars. On the basis of newly observed bipolar molecular outflows associated with massive stars, three properties are proposed to statistically identify massive stars whether in cluster or not as the driving engines of the flows. For clustering massive stars with some exceptions, their outflow collimation factors are generally poor and less than two, and the correlations of the flow momentum rate and the mass flow rate with the central source bolometric luminosity deviate the ones for selected well-resolved 16 flows.

Affiliated with

Also associated with

No associations

Rating

Outflows of Massive Stars in Cluster 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 Outflows of Massive Stars in Cluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Outflows of Massive Stars in Cluster will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1603532