High Velocity Gas Outflows from H II regions in Disc Galaxies

Details High Velocity Gas Outflows from H II regions in Disc Galaxies High Velocity Gas Outflows from H II regions in Disc Galaxies

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjas...3..181r&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, Supplement, p. 181-185

Astronomy and Astrophysics

Astrophysics

Hii Regions, Ism: Jets And Outflows, Stars: Mass Loss

Scientific paper

We analyze the Hα emission line profiles of the HII region populations in three disc spiral galaxies and find evidence of wing features at 40-90 km/s from the central peak in a significant fraction of regions. We explain the wing features as due to a shell expanding inside the HII region, quantify the energy involved and present two possible mechanisms to drive the expanding shell.

Affiliated with

Also associated with

No associations

Rating

High Velocity Gas Outflows from H II regions in Disc Galaxies 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 High Velocity Gas Outflows from H II regions in Disc Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Velocity Gas Outflows from H II regions in Disc Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-878644