2010A&A...510A..37M


Query : 2010A&A...510A..37M

2010A&A...510A..37M - Astronomy and Astrophysics, volume 510, A37-37 (2010/2-1)

Polycyclic aromatic hydrocarbon processing in a hot gas.

MICELOTTA E.R., JONES A.P. and TIELENS A.G.G.M.

Abstract (from CDS):

PAHs are thought to be a ubiquitous and important dust component of the interstellar medium. However, the effects of their immersion in a hot (post-shock) gas have never before been fully investigated. We study the effects of energetic ion and electron collisions on PAHs in the hot post-shock gas behind interstellar shock waves. We calculate the ion-PAH and electron-PAH nuclear and electronic interactions, above the carbon atom loss threshold, in Hii regions and in the hot post-shock gas for temperatures ranging from 103-108K. PAH destruction is dominated by He collisions at low temperatures (T<3x104K), and by electron collisions at higher temperatures. Smaller PAHs are destroyed faster for T<106K, but the destruction rates are roughly the same for all PAHs at higher temperatures. The PAH lifetime in a tenuous hot gas (nH≃0.01cm–3, T≃107K), typical of the coronal gas in galactic outflows, is found to be about thousand years, orders of magnitude shorter than the typical lifetime of such objects. In a hot gas, PAHs are principally destroyed by electron collisions and not by the absorption of X-ray photons from the hot gas. The resulting erosion of PAHs occurs via C2 loss from the periphery of the molecule, thus preserving the aromatic structure. The observation of PAH emission from a million degree, or more, gas is only possible if the emitting PAHs are ablated from dense, entrained clumps that have not yet been exposed to the full effect of the hot gas.

Abstract Copyright:

Journal keyword(s): shock waves - dust, extinction - ISM: jets and outflows

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17416 0
2 SNR J052501-693842 SNR 05 25 02.3 -69 38 39           ~ 401 1
3 M 42 HII 05 35 17 -05 23.4           ~ 4071 0
4 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 5852 6
5 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1612 0

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