An optical and H I study of late-type low surface brightness galaxies

Details An optical and H I study of late-type low surface brightness galaxies An optical and H I study of late-type low surface brightness galaxies

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.200..325l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 200, July 1982, p. 325-346.

Astronomy and Astrophysics

Astronomy

58

Astronomical Catalogs, Astronomical Spectroscopy, Brightness Distribution, Galactic Structure, H Lines, Surface Properties, Galactic Clusters, Hydrogen Ions, Light (Visible Radiation), Mass Distribution, Neutral Gases, Photographic Plates, Schmidt Telescopes, Spatial Distribution

Scientific paper

Neutral hydrogen and optical parameters are presented for 151 galaxies of low surface brightness selected from UK Schmidt plates. The 21-cm H I line was detected in 100 of these systems. It is found that the galaxies show the same trends of global properties with type as samples of bright galaxies, while the data are consistent with the low surface brightness (LSB) galaxies being of systematically lower mass than bright galaxies of the same type and linear dimensions. A constant value of hydrogen mass/(linear dimension)/squared is strongly suggested for LSB and bright galaxies.

Affiliated with

Also associated with

No associations

Rating

An optical and H I study of late-type low surface brightness 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 An optical and H I study of late-type low surface brightness galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An optical and H I study of late-type low surface brightness galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1024256