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| Query : 1996A&A...315L.337V |
1996A&A...315L.337V - Astronomy and Astrophysics, volume 315L337-340 (1996/11-2)
SWS spectroscopy of small grain features across the M17-Southwest photodissociation front.
VERSTRAETE L., PUGET J.L., FALGARONE E., DRAPATZ S., WRIGHT C.M. and TIMMERMANN R.
Abstract (from CDS):
We present SWS spectra taken across the M17-Southwest photodissociation front and discuss spectral properties of PAHs and VSGs. We report new features at 4.65, 6.35, 8.7 and 11µm which we interpret as PAHs and/or VSGs emission. From feature intensity ratios along the cut, we find PAHs are mainly ionized and almost fully hydrogenated.
Abstract Copyright: ∼
Journal keyword(s): ISM: molecules - ISM: dust - ISM: molecular cloud, HII region
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | NAME M 17 SW | SFR | 18 20 23.1 | -16 11 43 | ~ | 281 | 0 | |||||
| 2 | NGC 6618 | OpC | 18 20 47 | -16 10.3 | ~ | 1700 | 0 |
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