2019MNRAS.483.3574S

Query : 2019MNRAS.483.3574S

2019MNRAS.483.3574S - Mon. Not. R. Astron. Soc., 483, 3574-3578 (2019/March-1)

Formation of the NH molecule and its isotopologues through radiative association.

SZABO P. and GUSTAFSSON M.

Abstract (from CDS):

The rate coefficients and the cross-sections for the formation of imidogen (NH) molecule (and its isotopologues: 15NH and ND) through radiative association are determined by employing quantum mechanical perturbation theory, classical Larmor formula, and Breit-Wigner theory. We suggest the radiative association process as possible route for NH production in diffuse interstellar clouds.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): molecular processes - scattering - ISM: atoms - ISM: clouds - ISM: molecules

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 7

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Number of rows : 7
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 * zet Per s*b 03 54 07.9224751 +31 53 01.081262 2.19 2.97 2.85 2.71 2.62 B1Ib 881 0
2 * 62 Tau * 04 23 59.7627483096 +24 18 03.527065188 6.18 6.499 6.337     B3V 237 0
3 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
4 * zet Oph Be* 16 37 09.5400587698 -10 34 01.509742704 1.73 2.58 2.56 2.46 2.50 O9.2IVnn 1908 0
5 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
6 W 31c HII 18 10 29.1 -19 56 05           ~ 357 0
7 W 49n HII 19 10 13.2 +09 06 12           ~ 497 3

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