Chemistry of C<sub>2</sub>S and C<sub>3</sub>S in L1544 with NSRT

Abstract Sulfur-bearing species are widely utilized to investigate the physical structure of star-forming regions in interstellar media; however, the underlying sulfur chemistry in these environments remains poorly understood. Therefore, further studies of S-bearing species are fundamentally important, as they can enhance our understanding of the physical evolution of star-forming regions. This study presents observations of C 2 S and C 3 S in L1544, acquired using the Nanshan 26-m radio telescope, along with simulations of their chemical behavior using a one-dimensional physical model. The simulation results reveal significant radial variations in the column densities of C 2 S and C 3 S. Additionally, the column densities of both molecules are found to be sensitive to the cosmic ray ionization rate at several radial positions, while variations in the C/O ratio have comparatively minimal impact on L1544.

Authors

Institutions

Publication Details

Journal
Chinese Physics Letters
Published
2024-11-22
DOI
https://doi.org/10.1088/0256-307x/42/1/019701
Citations
1
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
0.33
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Chemistry of C2S and C3S in L1544 with NSRT

R. Szczerba, Xindi Tang, Jarken Esimbek, Gang Wu et al.
1 citations
Chinese Physics Letters
Astrophysics and Star Formation Studies
0.33
article

Chemistry of C2S and C3S in L1544 with NSRT

R. Szczerba, Xindi Tang, Jarken Esimbek, Gang Wu, Jixing Ge, Xuan Fang, Nadeem Iqbal, Donghui Quan, Jianjun Zhou, G. Fedoseev, Zhenzhen Miao, Chuan‐Lu Yang, Fangfang Li, Xia Zhang, Yong Zhang, Xiaohu Li, Rong Ma, Weiguang Ji, Yanan Feng, Yi-Han Wu, Tao Yang, Yuxin He, Juan Tuo
article en
1 citations

Abstract

Abstract Sulfur-bearing species are widely utilized to investigate the physical structure of star-forming regions in interstellar media; however, the underlying sulfur chemistry in these environments remains poorly understood. Therefore, further studies of S-bearing species are fundamentally important, as they can enhance our understanding of the physical evolution of star-forming regions. This study presents observations of C 2 S and C 3 S in L1544, acquired using the Nanshan 26-m radio telescope, along with simulations of their chemical behavior using a one-dimensional physical model. The simulation results reveal significant radial variations in the column densities of C 2 S and C 3 S. Additionally, the column densities of both molecules are found to be sensitive to the cosmic ray ionization rate at several radial positions, while variations in the C/O ratio have comparatively minimal impact on L1544.

Chinese Physics LettersVol. 42(1)
Sun Yat-sen University (CN), Ludong University (CN), Chinese Academy of Sciences (CN), Xinjiang Astronomical Observatory (CN), Zhejiang Lab (CN), Max Planck Institute for Radio Astronomy (DE), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), East China Normal University (CN), University of Hong Kong (HK)
Life below water
Openalex Percentile: Top 33%
Astrophysics and Star Formation Studies
0.33
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.