2008ApJ...679.1670H


Query : 2008ApJ...679.1670H

2008ApJ...679.1670H - Astrophys. J., 679, 1670-1679 (2008/June-1)

Calculations on the formation rates and mechanisms for cn H anions in interstellar and circumstellar media.

HERBST E. and OSAMURA Y.

Abstract (from CDS):

The rate coefficients for the radiative attachment reactions between the radicals Cn H (n=2-8) and electrons have been calculated with the aid of quantum chemistry using a phase-space theory in which strong coupling exists among the ground and any excited anion electronic states with the same spin. The results confirm that the process increases in efficiency with the size of the radical. For n≥6, the rate coefficients lie at the collisional limit, in agreement with earlier estimates. For n=4,5, the new results are larger than the old estimates. The calculated rate coefficient for C4H+e– is now much too large to explain the current observed abundance ratio of C4H–/C4 H in IRC +10216 and L1527 and its upper limit in TMC-1. It is quite possible that electronic coupling is weak, and that so-called ``dipole-bound'' and other states must act as doorways to radiative attachment. We have also calculated potential surfaces for dissociative attachment starting with the ``carbenes'' H2C_2m_(m=2-4) and leading to the syntheses of the anions C_2m_H–.

Abstract Copyright: ∼

Journal keyword(s): Astrochemistry - ISM: Abundances - ISM: Molecules

Simbad objects: 4

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Number of rows : 4
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 LDN 1527 DNe 04 39 53 +25 45.0           ~ 689 0
2 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
3 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2455 0
4 * 23 Leo * 09 51 01.9840280136 +13 03 58.460768316 9.970 8.030 6.450 10.9   M0III 47 0

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