Published December 15, 1989 | Version v1
Journal article

HAC-coated silicate grains and PAHs in diffuse clouds and low-velocity shocks

  • 1. Toronto Univ., ON (Canada). Canadian Inst. for Theoretical Astrophysics
  • 2. York Univ., Toronto, ON (Canada). Dept. of Physics
  • 3. Manchester Univ. (UK). Inst. of Science and Technology

Description

We investigate a model in which HAC-coated silicate grains subjected to low-velocity shocks release carbon to the gas in the form of atoms and PAHs. Both HAC and PAH are assumed to be subject to chemistry, including reactions with oxygen atoms, carbon atoms and carbon ions. The released species contribute to a conventional post-shock chemistry, during which the HAC and PAHs may be further eroded or restored. We find that the parameter of crucial importance is the reaction efficiency for atomic oxygen with both HAC and PAH. If this efficiency is less than 100 per cent, then HAC mantles are (at least) restored in a period of about 106 yr. PAHs are destroyed on time-scales of less than about 105 yr unless the oxidation efficiency is very small. (author)

Additional details

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
241
Journal Issue
4
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
753-767
ISSN
0035-8711
CODEN
MNRAA

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
21029815
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
AMORPHOUS STATE; CARBON; CHEMICAL REACTIONS; COATINGS; COSMOCHEMISTRY; HYDROGEN COMPOUNDS; INTERSTELLAR GRAINS; NEBULAE; SHOCK WAVES; SILICATES
Descriptors DEC
CHEMISTRY; ELEMENTS; NONMETALS; OXYGEN COMPOUNDS; PARTICLES; SILICON COMPOUNDS