Analysis of galaxy neutral hydrogen spectra

Details Analysis of galaxy neutral hydrogen spectra Analysis of galaxy neutral hydrogen spectra

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73...37n&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. 37-39

Astronomy and Astrophysics

Astrophysics

Galactic Radiation, Galactic Structure, H Lines, Line Shape, Neutral Gases, Autocorrelation, Line Spectra, Molecular Rotation

Scientific paper

The 21 cm spatially integrated neutral hydrogen line profile observed in nearby galaxies contains significant information about the distribution of neutral hydrogen. It is shown, for a standard model of galactic structure (azimuthally symmetric, thin disk), that the neutral hydrogen distribution as a function of rotation velocity can be calculated directly from either the spectral line shape or the corresponding autocorrelation function.

Affiliated with

Also associated with

No associations

Rating

Analysis of galaxy neutral hydrogen spectra 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 Analysis of galaxy neutral hydrogen spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of galaxy neutral hydrogen spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648774