2012ApJ...752..159R


Query : 2012ApJ...752..159R

2012ApJ...752..159R - Astrophys. J., 752, 159 (2012/June-3)

Radiation synthesis of carbon dioxide in ice-coated carbon: implications for interstellar grains and icy moons.

RAUT U., FULVIO D., LOEFFLER M.J. and BARAGIOLA R.A.

Abstract (from CDS):

We report the synthesis of carbon dioxide on an amorphous carbon-13 substrate coated with amorphous water ice from irradiation with 100 keV protons at 20 K and 120 K. The quantitative studies show that the CO2 is dispersed in the ice; its column density increases with ion fluence to a maximum value (in 1015 molecules/cm2) of ∼1 at 20 K and ∼3 at 120 K. The initial yield is 0.05 (0.1) CO2 per incident H+ at 20 (120) K. The CO2destruction process, which limits the maximum column density, occurs with an effective cross section of ∼2.5 (4.1)x10–17 cm2 at 20 (120) K. We discuss radiation-induced oxidation by reactions of radicals in water with the carbon surface and demonstrate that these reactions can be a significant source of condensed carbon dioxide in interstellar grains and in icy satellites in the outer solar system.

Abstract Copyright: ∼

Journal keyword(s): astrochemistry - ISM: abundances - ISM: molecules - methods: laboratory - planets and satellites: composition - planets and satellites: surfaces

Simbad objects: 2

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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 W 33a Y*O 18 14 39.56547 -17 52 02.2260           ~ 746 0
2 NAME SH 2-140 IRS 1 Y*O 22 19 18.277 +63 18 45.82           ~ 201 0

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