arrow
Return

Predicting reliable H2 column density maps from molecular line data using machine learning

delete2023-09-11
delete0
delete
OA
AI
Y
Yoshito Shimajiri *
Y
Yasutomo Kawanishi
S
Shinji Fujita
Y
Yusuke Miyamoto
A
Atsushi Ito
D
D. Arzoumanian
P
P. André
A
Atsushi Nishimura
K
Kazuki Tokuda
H
Hiroyuki Kaneko
S
Shunya Takekawa
S
Shota Ueda
T
Toshikazu Onishi
T
Tsuyoshi Inoue
S
Shimpei Nishimoto
R
Ryuki Yoneda
DOI:10.1093/mnras/stad2715delete
deleteOriginal
deleteOriginal request for help
deleteShare
deleteSave
Abstract

Abstract

En 中文
The total mass estimate of molecular clouds suffers from the uncertainty in the H-2-CO conversion factor, the so-called X-CO factor, which is used to convert the (CO)-C-12 (1-0) integrated intensity to the H-2 column density. We demonstrate the machine learning's ability to predict the H-2 column density from the (CO)-C-12, (CO)-C-13, and (CO)-O-18 (1-0) data set of four star-forming molecular clouds: Orion A, Orion B, Aquila, and M17. When the training is performed on a subset of each cloud, the overall distribution of the predicted column density is consistent with that of the Herschel column density. The total column density predicted and observed is consistent within 10 per cent, suggesting that the machine learning prediction provides a reasonable total mass estimate of each cloud. However, the distribution of the column density for values >similar to 2 x 10(22)cm(-2), which corresponds to the dense gas, could not be predicted well. This indicates that molecular line observations tracing the dense gas are required for the training. We also found a significant difference between the predicted and observed column density when we created the model after training the data on different clouds. This highlights the presence of different X-CO factors between the clouds, and further training in various clouds is required to correct for these variations. We also demonstrated that this method could predict the column density towards the area not observed by Herschel if the molecular line and column density maps are available for the small portion, and the molecular line data are available for the larger areas.
Keywords:
methods: statistical
ISM: abundances
ISM: clouds
ISM: molecules

Journal

Monthly Notices of the Royal Astronomical Society cover
Monthly Notices of the Royal Astronomical Society
IF:
4.8
Papers:
7.0W
Citations:
25.0W

Organization

U
University of Tokyo
Scholars:
7.1W
Papers: 6.5W
Citations: 2.2K
C
centre national de la recherche scientifique (cnrs)
Scholars:
24.5W
Papers: 18.2W
Citations: 279
N
national institutes of natural sciences (nins) - japan
Scholars:
8.6K
Papers: 9.1K
Citations: 3
C
CEA
Scholars:
3.5W
Papers: 2.3W
Citations: 62
O
Osaka Metropolitan University
Scholars:
1.2W
Papers: 9.7K
Citations: 1.6K
Fukui University of Technology cover
Fukui University of Technology
Scholars:
158
Papers: 184
Citations: 140
K
kyushu kyoritsu university
Scholars:
51
Papers: 37
Citations: 0
N
national institute for fusion science (nifs) - japan
Scholars:
708
Papers: 532
Citations: 0
R
riken
Scholars:
2.2W
Papers: 1.9W
Citations: 24
researcher View more organizations