Emission lines due to interstellar dust in the visible spectra of nebulae

Details Emission lines due to interstellar dust in the visible spectra of nebulae Emission lines due to interstellar dust in the visible spectra of nebulae

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..61..243d&link_type=abstract

Astrophysics and Space Science, vol. 61, no. 1, Mar. 1979, p. 243-246. Research supported by the National Research Council of C

Astronomy and Astrophysics

Astrophysics

2

Emission Spectra, Interstellar Matter, Light (Visible Radiation), Line Spectra, Planetary Nebulae, Calcium Oxides, Chromium, Fluorescence, Magnesium Oxides, Phonons

Scientific paper

It is suggested that certain sharp lines in the visible and
near-ultraviolet spectra of nebulae may be due to fluorescence from
grains. Evidence is presented that some of these lines could arise from
MgO or CaO grains. Some sharp diffuse interstellar bands may also appear
in the spectra of nebulae.

Affiliated with

Also associated with

No associations

Rating

Emission lines due to interstellar dust in the visible spectra of 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 Emission lines due to interstellar dust in the visible spectra of nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission lines due to interstellar dust in the visible spectra of nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1649037