Properties of young clusters near reflection nebulae

Details Properties of young clusters near reflection nebulae Properties of young clusters near reflection nebulae

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8325628s&link_type=abstract

Unknown

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Early Stars, Reflection Nebulae, Star Clusters, Stellar Luminosity, Hydrogen, Infrared Spectra, Open Clusters, Spatial Distribution, Stellar Mass, Stellar Spectrophotometry

Scientific paper

Near infrared observations in the reflection nebulae NGC 7023, 2023, and 2068 are used to study clusters of young stars found associated with these nebulae. At least 30% to 60% of these stars are pre-main sequence objects, as indicated by their infrared excesses, hydrogen line emission, or irregular variability. The spatial distributions and observed luminosity functions of these young open clusters are derived, and the inferred mass function and star formation efficiencies are discussed.

Affiliated with

Also associated with

No associations

Rating

Properties of young clusters near reflection nebulae 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 Properties of young clusters near reflection nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of young clusters near reflection nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1587608