Infrared spectrophotometry of M 17 with ISOCAM.

Details Infrared spectrophotometry of M 17 with ISOCAM. Infrared spectrophotometry of M 17 with ISOCAM.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...315l.309c&link_type=abstract

Astronomy and Astrophysics, v.315, p.L309-L312

Astronomy and Astrophysics

Astrophysics

141

Ism: Individual: M 17, Ism: Dust, Ism: Molecules, Ism: Atoms, Infrared: Ism: Lines And Bands, Infrared: Ism: Continuum

Scientific paper

We report spectrophotometric observations of the HII region/neutral medium interface in M 17 obtained with the ISOCAM Circular Variable Filter (CVF) in the spectral range 5.15 to 16.5μm. The lines of singly-ionized species come mainly from the clumpy "neutral" interface, while the HII region dominates the line emission by higher-ionization species. The emission in the Unidentified Infrared Bands (UIBs) comes from the molecular cloud and the interface and extends into the HII region. In the regions where the radiation field is larger than about 10^4^ times the standard interstellar one, the continuum is dominated by the emission of very small grains which are bigger than those responsible for the UIBs.

Affiliated with

Also associated with

No associations

Rating

Infrared spectrophotometry of M 17 with ISOCAM. 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 Infrared spectrophotometry of M 17 with ISOCAM., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared spectrophotometry of M 17 with ISOCAM. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1145092