Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...364..723d&link_type=abstract
Astronomy and Astrophysics, v.364, p.723-731 (2000)
Astronomy and Astrophysics
Astrophysics
16
Scattering, Ism: Individual Objects: Sh 138, Ism: Dust, Extinction, Ism: H Ii Regions, Infrared: Ism: Lines And Bands
Scientific paper
We present visible and infrared images and low-dispersion visible spectra of the galactic compact H Ii region Sh 152. The spatial distribution of the Extended Red Emission (ERE) over the nebula is found to coincide with that of the ionized hydrogen emission and to differ from that of the Unidentified InfraRed Bands (UIRBs) emission at 3.3 and 6.2 mu m. This result and other considerations are in favour of grains as carriers of the ERE. It is shown that nanosized silicon particles could account for the ERE in terms of luminescence, an interpretation which, however, suffers from some limitations.
Darbon Stephane
Ducci V.
Perrin Jean-Marie
Savine C.
Sivan Jean-Pierre
No associations
LandOfFree
Extended red emission and unidentified infrared bands in the galactic compact H II region Sh 152 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 Extended red emission and unidentified infrared bands in the galactic compact H II region Sh 152, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extended red emission and unidentified infrared bands in the galactic compact H II region Sh 152 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1721990