H II region statistics in spirals

Details H II region statistics in spirals H II region statistics in spirals

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..297c&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

2

Astronomical Photometry, H Ii Regions, Spiral Galaxies, Stellar Luminosity, Telescopes, Accretion Disks, Electron Density (Concentration), Galactic Structure, H Alpha Line, Star Formation

Scientific paper

High-resolution maps of the spiral galaxies NGC 3992 and NGC 4321, obtained with the Taurus camera at the 4.2-m William Herschel Telescope are analyzed. The results obtained include (1) the total number of separately identifiable H II regions in their disks (classified according to their membership of a spiral arm or the interarm disk, (2) the radial distribution of H II regions, (3) the frequency distribution of diameters of H II regions, and (4) the luminosity function.

Affiliated with

Also associated with

No associations

Rating

H II region statistics in spirals 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 H II region statistics in spirals, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H II region statistics in spirals will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1124920