Computer Science
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982nyasa.395..165i&link_type=abstract
(NASA, National Science Foundation, New York Academy of Sciences, et al., Symposium on the Orion Nebula to Honor Henry Draper, N
Computer Science
1
Orion Constellation, Star Distribution, Stellar Evolution, Density Distribution, Orion Nebula, Stellar Radiation, Supernovae
Scientific paper
The types of compressing mechanisms needed to produce a star-forming process were investigated in the Orion region, where the stars are very young. It was determined that the stars in this region began to be formed by different triggering mechanisms. The characteristics of the distribution of stars in the different Orion regions were examined in order to determine which mechanism was dominant. Since the age of the stars in the Orion Nebula ranges from 10 to the 4th to 3 x 10 to the 7th years and the stellar components in regions in the Barnard Loop and outside the Loop are different, it was concluded that three types of triggering mechanisms are at work in the Orion region.
No associations
LandOfFree
Distribution of stars in the Orion region 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 Distribution of stars in the Orion region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distribution of stars in the Orion region will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1031785