1995A&A...299..835J


Query : 1995A&A...299..835J

1995A&A...299..835J - Astronomy and Astrophysics, volume 299835-846 (1995/7-3)

Infrared spectroscopy of gas-phase PAH molecules. II. Role of the temperature.

JOBLIN C., BOISSEL P., LEGER A., D'HENDECOURT L. and DEFOURNEAU D.

Abstract (from CDS):

Although it is now considered that the Unidentified IR (UIR) emission bands at 3.3, 6.2, 7.7, 8.6 and 11.3µm are due to aromatic hydrogenated compounds, there is more controversy over whether the carriers are free molecules, especially polycyclic aromatic hydrocarbons (PAHs), or are associated to larger dust particles. For example, the observed position of the 3.3µm band is better reproduced in laboratory by condensed molecules than by gas-phase molecules. On the other hand, free PAHs after the absorption of a single UV photon can easily reach the high temperatures (∼1000K) required to emit at 3.3µm. In this paper, we report the measurements of IR absorption bands of gas-phase PAHs at various temperatures up to about 1000K. The band positions clearly depend on the vibrational content of the molecules, which is interpreted in terms of anharmonic couplings. In the particular case of the 3.3µm band, it is found that the observed position for this band is consistent with the carriers being free PAHs at high temperatures. It is proposed that this feature is dominated by molecules of the size of coronene (C24H12) which absorb photons of mean energy 6eV and/or by larger molecules of typically 50 carbon atoms which are exposed to 10eV photons.

Abstract Copyright: ∼

Journal keyword(s): ISM: dust - ISM: molecules - molecular data - methods: laboratory - infrared: ISM: lines and bands

Simbad objects: 1

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Number of rows : 1
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 [D75b] Em* 21-021 PN 21 29 58.4711786760 +51 04 00.323924520   15.66 14.20 13.89   O7(f)/[WC11] 259 0

Query : 1995A&A...299..835J

Basic data :
[D75b] Em* 21-021 -- Planetary Nebula
Other object types:
otypes_help
PN (2013MNRAS,PN,...), Em* (HBHA,[D75b],...), * (UCAC4,[LFO93],...), MIR (MSX5C,WISEA,...), AB? (1991A&AS), NIR (2MASS), IR (IRAS)
ICRS coord. (ep=J2000) :
21 29 58.4711786760 +51 04 00.323924520 (Optical) [ 0.0169 0.0152 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
21 28 15.1113842661 +50 50 47.837315328 [ 0.0169 0.0152 90 ]
Gal coord. (ep=J2000) :
093.9873154875497 -00.1178059825260 [ 0.0169 0.0152 90 ]
Proper motions mas/yr :
-3.808 -2.445 [0.026 0.020 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.2677 [0.0185] A 2020yCat.1350....0G
Spectral type:
O7(f)/[WC11] C 1987ApJ...321L.151C
Fluxes (7) :
B 15.66 [0.07] D 2012yCat.1322....0Z
V 14.20 [0.04] D 2012yCat.1322....0Z
R 13.89 [0.13] E 2012yCat.1322....0Z
G 13.803763 [0.003300] C 2020yCat.1350....0G
J 11.504 [0.019] C 2003yCat.2246....0C
H 10.709 [0.017] C 2003yCat.2246....0C
K 9.551 [0.020] C 2003yCat.2246....0C
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Identifiers (15) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

PN G093.9-00.1 MSX5C G093.9873-00.1176 WISEA J212958.47+510400.3 [LFO93] 2128+50
HBHA 5203-13 PK 093-00 2 WISE J212958.42+510400.0 Gaia DR2 2171652769005709568
IRAS 21282+5050 TIC 64893572 [D75b] Em* 21-021 Gaia DR3 2171652769005709568
2MASS J21295847+5104002 UCAC4 706-083876 [KW97] 58-15

References (259 between 1850 and 2026) (Total 259)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 2    Plx : 2    PM : 2    SpT : 2   

   

Observing logs
Herschel : 9    ISO : 14   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : [D75b] Em* 21-021

Link by name to the catalogue in VizieR :

PN G093.9-00.1 IRAS 21282+5050 2MASS J21295847+5104002 MSX5C G093.9873-00.1176 UCAC4 706-083876
WISEA J212958.47+510400.3 WISE J212958.42+510400.0 Gaia DR2 2171652769005709568 Gaia DR3 2171652769005709568

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