Near-Infrared Luminosity Functions of Young Clusters

Details Near-Infrared Luminosity Functions of Young Clusters Near-Infrared Luminosity Functions of Young Clusters

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.6601l&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #66.01; Bulletin of the American Astronomical Society, Vol. 27, p.1376

Astronomy and Astrophysics

Astronomy

Scientific paper

Young clusters provide us with an unique opportunity to study the process of stars formation and early stellar evolution in a statistically significant manner. In particular, investigations and comparisons of the luminosity functions of very young clusters should provide important constraints on the shape and universality of the IMF. In my talk, I will present and compare the near-infrared luminosity functions for several nearby clusters. In addition, evolutionary models for the near-infrared luminosity functions of such clusters will be used to constrain their star formation history.

Affiliated with

Also associated with

No associations

Rating

Near-Infrared Luminosity Functions of Young Clusters 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 Near-Infrared Luminosity Functions of Young Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-Infrared Luminosity Functions of Young Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1254822