The formation and destruction of HeH/+/ in astrophysical plasmas

Details The formation and destruction of HeH/+/ in astrophysical plasmas The formation and destruction of HeH/+/ in astrophysical plasmas

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255..489r&link_type=abstract

Astrophysical Journal, Part 1, vol. 255, Apr. 15, 1982, p. 489-496.

Astronomy and Astrophysics

Astrophysics

84

Cosmic Plasma, Helium Ions, Hydrogen Ions, Molecular Clouds, Planetary Nebulae, Abundance, Association Reactions, Dense Plasmas, Emission Spectra, Extreme Ultraviolet Radiation, Hydrogen Clouds, Ionization, Molecular Excitation, Molecular Interactions, Molecular Ions, Photodissociation, Recombination Reactions, X Rays

Scientific paper

A discussion is presented of the formation and destruction mechanisms of the molecular ion HeH(+) in astrophysical plasmas. Calculations are made of the steady state abundance of HeH(+) in planetary nebulae and in dense clouds subjected to X-ray and XUV ionization. The excitation processes are investigated, and estimates are made of the emission-line intensities at 149.13, 3.364, and 3.607 microns. Emission at 149.13 microns from H II blisters and at 3.364 microns from high density planetary nebulae may be detectable.

Affiliated with

Also associated with

No associations

Rating

The formation and destruction of HeH/+/ in astrophysical plasmas 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 The formation and destruction of HeH/+/ in astrophysical plasmas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The formation and destruction of HeH/+/ in astrophysical plasmas will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-840702