Equivalent Width of Interstellar Molecular Lines. IV: Analyses of the Line Spectrum of H2 in the Interstellar Spectrum of δ Scorpii

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We have made an analysis of the observed equivalent widths of the lines of Lyman and Werner bands by Smith. The H2 column densities of 3×1019 to 1020 and the excitation temperature of 80 to 150 K satisfy the observations. This temperature refers to the kinetic temperature. We have also discussed the importance of getting the excitation temperature from lines of H2 and other heteronuclear diatomic molecules for the same star and from different regions of space.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Equivalent Width of Interstellar Molecular Lines. IV: Analyses of the Line Spectrum of H2 in the Interstellar Spectrum of δ Scorpii 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 Equivalent Width of Interstellar Molecular Lines. IV: Analyses of the Line Spectrum of H2 in the Interstellar Spectrum of δ Scorpii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equivalent Width of Interstellar Molecular Lines. IV: Analyses of the Line Spectrum of H2 in the Interstellar Spectrum of δ Scorpii will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1839972

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.