An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules

Details An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.166..333w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 166, no. 2, April 1990, p. 333-335.

Astronomy and Astrophysics

Astrophysics

2

Aromatic Compounds, Infrared Spectra, Planetary Nebulae, Stellar Composition, Emission Spectra, Interstellar Extinction, Molecular Spectra

Scientific paper

It was recently pointed out that an ensemble of aromatic molecules derived from natural products would account for both the shape of the 3.3 micron emission feature in NGC2023 and the 2200 A absorption in the interstellar extinction curve. Here, the expected emission features from an ensemble of naturally-occurring aromatic molecules is shown to be in satisfactory agreement with the emission properties of PAH molecules associated with PN.

Affiliated with

Also associated with

No associations

Rating

An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules 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 An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An integrated 2.5-12.5 micron emission spectrum of naturally-occurring aromatic molecules will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1379887