The kinematics of giant extragalactic H II regions

Details The kinematics of giant extragalactic H II regions The kinematics of giant extragalactic H II regions

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280..580s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 280, May 15, 1984, p. 580-591.

Astronomy and Astrophysics

Astrophysics

44

Galactic Structure, H Ii Regions, Kinematics, Nebulae, Astronomical Maps, Emission Spectra, Stellar Winds, Supernovae, Visible Spectrum

Scientific paper

The kinematic structures of giant extragalactic H II regions in spiral galaxies, irregular galaxies, and "isolated extragalactic H II regions" are studied. Line profiles were found to be broad (FWHM > 30 km s-1) throughout the core. Every region studied contains at least one "nucleus" with bright and, perhaps surprisingly, narrow emission lines. These data are discussed with regard to previous explanations for the large line widths observed in giant extragalactic H II regions.

Affiliated with

Also associated with

No associations

Rating

The kinematics of giant extragalactic H II regions 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 The kinematics of giant extragalactic H II regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The kinematics of giant extragalactic H II regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1368091