Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232l..53s&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 232, Aug. 15, 1979, p. L53-L57.
Astronomy and Astrophysics
Astronomy
80
Absorption Spectra, Carbon Monoxide, Infrared Astronomy, Infrared Spectrophotometers, Interstellar Matter, Radiation Sources, Graphs (Charts), Silicates, Tables (Data)
Scientific paper
The spectrum of the highly obscured infrared source W33 A from 4.5 to 8 microns is measured in order to investigate the intervening cold, dense interstellar material. Spectrophotometry at a relative spectral resolution of about 0.015 by an airborne filter-wheel infrared spectrometer reveals strong absorption features at 4.61, 5.99 and 6.78 microns. The absorption at 4.61 microns is attributed primarily to the fundamental vibration-rotation band of CO at a column density (at least 10 to the 19th/sq cm) which is 10% of the carbon inferred from silicate abundances. The strengths and line widths of the absorption agt 5.99 and 6.78 microns are interpreted as evidence of absorption in the resonance bands of carbonyl, carbon-carbon double, methyl and methylene bonds of hydrocarbons associated with interstellar dust.
Gillett Fred C.
Harvey Paul Michael
Puetter Richard C.
Russell Ray W.
Soifer Thomas B.
No associations
LandOfFree
The 4-8 micron spectrum of the infrared source W33 A 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 4-8 micron spectrum of the infrared source W33 A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 4-8 micron spectrum of the infrared source W33 A will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1483829