Interstellar molecular absorption lines

Details Interstellar molecular absorption lines Interstellar molecular absorption lines

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rspta.279..323d&link_type=abstract

(Royal Society, Discussion on Astronomy in the Ultraviolet, London, England, Apr. 9, 10, 1974.) Royal Society (London), Philosop

Astronomy and Astrophysics

Astronomy

1

Interstellar Extinction, Line Spectra, Molecular Absorption, Stellar Radiation, Ultraviolet Absorption, Absorption Spectra, Early Stars, Molecular Spectra, Nebulae, Radiative Lifetime

Scientific paper

The ultraviolet absorption lines produced in interstellar clouds through the absorption of radiation from early-type stars by molecular hydrogen may be analyzed to yield the particle densities and ultraviolet fluxes in the absorbing regions. The absorption by HD may be analyzed to determine the proton densities and the ionizing fluxes. The interpretation carries implications concerning the formation of other interstellar molecules, which may be the source of additional absorption lines.

Affiliated with

Also associated with

No associations

Rating

Interstellar molecular absorption lines 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 Interstellar molecular absorption lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar molecular absorption lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1757444