Formation and Evolution of Molecules Behind Shocks
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Transcript of Formation and Evolution of Molecules Behind Shocks
Formation and Evolution of Molecules Behind Shocks
GEORGE HASSEL Dept. of Physics, The Ohio State University
Eric Herbst (Ohio State), Ted Bergin (U. Michigan)SATURDAY, NOVEMBER 8, 2008 MWAM’08
OVERVIEW
• Can shocks form dense clouds from diffuse ISM? (Bergin et al. 2004)
• Replicate molecular observations?
– Ice composition with AV (Whittet et al. 2007, Nummelin et al. 2001)
– Complex gas molecules: L134N, TMC-1 (Ohishi et al 1992, Wakelam, Herbst & Selsis 2007)
Modifications:
• Read shock hydro results as input
• Compute dust temperature
• New / modified rates:– Photodesorption
– Eley-Rideal
– CO + O surface barrier
OSU GAS-GRAIN NETWORK
Grain Model: r = 0.1 m Spherical, silicate grains
Rate equations – no stochastic methods
Shock Chemistry Model• Hydrodynamical 1 point model (Bergin et al. 2004)
• Diffuse ISM -> Shock -> Dense cloud?
• Formation of H2(g) & CO(g) - ices & complex species?
Photos from NASA-APOD Archive
Physical Conditions
• nH, Tg – dense cloud ~105-6 yr
• AV, Td – more gradual change
Photodesorption Rates
CO:
Direct photodesorption
Temperature dependent
CO2:
Photodissociation / desorption
Temperature, coverage dependentN2:
Direct photodesorption only with CO
**indicates non-thermal**
H2O:
Photodissociation / desorption
Oberg et al. 2007, in prep.
Ice – No Photodesorption
Ices: Whittet et al. 2007, CO(g): Ohishi et al 1992 (TMC-1, L134N)
Ice – Photodesorption
Ice Composition
• Formation at AV ~ 3-4
OH(s) + H(s) -> H2O(s)
CO(g) -> CO(s)
Ice Composition
CO(s) + OH(s) -> CO2(s)
CO2(s) + h -> CO(s) + O(s)
CO(s) + O(s) -> CO2(s)
EA = 290 K (Roser et al. 2001)
= 130 K (Ruffle & Herbst 2001)
CO2 Ice
Td0=20 K
EA= 130 K
EA=290 K
Td0=15 K
EA= 130 K
EA=290 K
Complex Gas Molecules
H2S NH3
HC3N
14 species
6 species
17-29 species
Conclusions• Ice composition:
H2O : CO : CO2 ~ observed abundances
AV Threshold
CH4 minimized
• Governed by photodesorption
• Gas phase molecules – 3 distinct evolution stages
Acknowledgements
• Rob Garrod
• Herma Cuppen & Karin Oberg
• MWAM ’08 Organizing Committee