Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae

Details Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...305..399s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 305, June 1, 1986, p. 399-404.

Astronomy and Astrophysics

Astrophysics

50

Emission Spectra, Filter Wheel Infrared Spectrometers, Fluorescence, Hydrogen, Nebulae, B Stars, Molecular Spectroscopy, Ultraviolet Reflection, Vibrational Spectra

Scientific paper

Strong molecular hydrogen emission at 2.41 μm has been observed in three out of six reflection nebulae surveyed. A spectrum of one nebula, Parsamyan 18, shows several H2 lines whose intensity ratios have values agreeing with those predicted if the excitation is due to UV-pumped fluorescence and disagreeing with those predicted for shock and X-ray excitations.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae 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 Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet-pumped infrared fluorescent molecular hydrogen emission in reflection nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1830214