Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1968
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968ap%26ss...2..461d&link_type=abstract
Astrophysics and Space Science, Volume 2, Issue 4, pp.461-473
Astronomy and Astrophysics
Astrophysics
25
Scientific paper
The collision of supersonic gas streams within an HII region is studied. A system of stationary shock waves is set up. Theoretical line profiles through these shocked regions are compared with those obtained in the bright central regions of the Orion Nebula. There is good agreement between the predicted and observed magnitude of line splitting in the forbidden lines of O+ and O++.
No associations
LandOfFree
Dynamics of the Orion Nebula. II: Shock Waves in an H II 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 Dynamics of the Orion Nebula. II: Shock Waves in an H II Region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of the Orion Nebula. II: Shock Waves in an H II Region will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1361963