Spectroscopy of the 3 micron emission features

Details Spectroscopy of the 3 micron emission features Spectroscopy of the 3 micron emission features

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..500g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 15, 1985, p. 500-505. NSF-NASA-supported research.

Astronomy and Astrophysics

Astronomy

91

Astronomical Spectroscopy, Emission Spectra, Infrared Astronomy, Planetary Nebulae, H Ii Regions, High Resolution, Line Spectra, Spectral Resolution, Stellar Mass Ejection

Scientific paper

High-spectral-resolution observations of the 3.3 and 3.4 microns features in the three planetary nebulae NGC 7027, IC 418, and BD +30 deg 3639, in the H II region S106, and in the 'red rectangle' HD 44179 are presented. The profile of the unidentified 3.3 microns emission feature is similar in all five sources. The unidentified feature previously referred to as the 3.4 microns feature actually consists of two components, a low-level emission from 3.35 to 3.60 microns and a narrow emission peak at 3.40 microns. The strength of the latter feature relative to that of the 3.3 microns feature varies by a a factor of three from source to source. The origin and properties of these features may be explained by further development of the small-grain models of Sellgren (1984) and Leger and Puget (1984).

Affiliated with

Also associated with

No associations

Rating

Spectroscopy of the 3 micron emission features 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 Spectroscopy of the 3 micron emission features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopy of the 3 micron emission features will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1631278