2022RAA....22a5004G


Query : 2022RAA....22a5004G

2022RAA....22a5004G - Research in Astron. and astroph., 22, part no 1, 5004-15004 (2022/January-0)

GGCHEMPY: A Pure Python-based Gas-grain Chemical Code for Efficient Simulation of Interstellar Chemistry.

GE J.

Abstract (from CDS):

In this paper, we present a new gas-grain chemical code for interstellar clouds written in pure Python (GGCHEMPY (GGCHEMPY is available on https://github.com/JixingGE/GGCHEMPY)). By combining with the high-performance Python compiler Numba, GGCHEMPY is as efficient as the Fortran-based version. With the Python features, flexible computational workflows and extensions become possible. As a showcase, GGCHEMPY is applied to study the general effects of three-dimensional projection on molecular distributions using a two-core system which can be easily extended for more complex cases. By comparing the molecular distribution differences between two overlapping cores and two merging cores, we summarized the typical chemical differences such as N2H+, HC3N, C2S, H2CO, HCN and C2H, which can be used to interpret 3D structures in molecular clouds.

Abstract Copyright: © 2022 National Astronomical Observatories

Journal keyword(s): astrochemistry - (ISM:) evolution - ISM: molecules - ISM: abundances - methods: numerical

Simbad objects: 9

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Number of rows : 9
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 1495 DNe 04 18.1 +27 37           ~ 408 1
2 PLCKECC G168.72-15.48 cor 04 18 34.6 +28 26 35           ~ 10 0
3 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
4 LDN 1544 DNe 05 04 16.6 +25 10 48           ~ 965 0
5 NAME lam Ori Cloud Cld 05 35 06 +09 56.0           ~ 76 0
6 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
7 NAME Ori B MoC 05 41 43.0 -01 54 44           ~ 1498 0
8 PLCKECC G224.47-00.65 cor 07 10 21.7 -10 33 30           ~ 10 0
9 LDN 1147 DNe 20 40 32 +67 20.7           ~ 35 0

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