Exploring Sulfur Chemistry in TMC-1 with NSRT

被引:0
作者
Wasim Iqbal [1 ,2 ]
Xiaohu Li [1 ,2 ,3 ]
Juan Tuo [1 ,4 ]
Ryszard Szczerba [1 ,2 ,5 ]
Yanan Feng [1 ,4 ]
Zhenzhen Miao [1 ,2 ]
Jiangchao Yang [1 ,4 ]
Jixing Ge [1 ,2 ]
Gleb Fedoseev [1 ,2 ,6 ]
Donghui Quan [7 ,1 ]
Qiang Chang [8 ]
Chuan-Lu Yang [1 ,9 ]
Tao Yang [1 ,10 ]
Gao-Lei Hou [11 ]
Yong Zhang [1 ,12 ,13 ]
Xuan Fang [1 ,14 ,13 ]
Xia Zhang [1 ,2 ]
Fangfang Li [1 ,2 ,4 ]
Rong Ma [1 ,4 ]
Xiaomin Song [1 ,4 ]
Zhiping Kou [1 ,4 ]
Yuxuan Sun [1 ,4 ]
机构
[1] State Key Laboratory of Precision Spectroscopy, East China Normal University
[2] MOE Key Laboratory for Non-Equilibrium Synthesis and Modulation of Condensed Matter, School of Physics,Xi’an Jiaotong University
[3] School of Physics and Astronomy, Sun Yat-sen University
[4] Laboratory for Space Research, Faculty of Science, The University of Hong Kong
[5] National Astronomical Observatories, Chinese Academy of Sciences
[6] Xinjiang Astronomical Observatory, Chinese Academy of Sciences
[7] Xinjiang Key Laboratory of Radio Astrophysics
[8] Key Laboratory of Radio Astronomy, Chinese Academy of Sciences
[9] University of Chinese Academy of Sciences
[10] Nicolaus Copernicus Astronomical Center
[11] Research Laboratory for Astrochemistry, Ural Federal University
[12] Astronomical Computing Research Center, Zhejiang Laboratory
[13] School of Physics and Optoelectronic Engineering, Shandong University of Technology
[14] School of Physics and Optoelectronic Engineering, Ludong University
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中图分类号
P148 [天体化学];
学科分类号
070401 ;
摘要
There have been several studies on sulfur depletion in dense cores like TMC-1(Taurus Molecular Cloud1), employing updated reaction networks for sulfur species to explain the missing sulfur in the gas within dense clouds. Most of these studies used a C/O ratio of 0.7 or lower. We present NSRT(NanShan 26m Radio Telescope)observations of TMC-1 alongside results from time-dependent chemical simulations using an updated chemical network. Our findings highlight the impact of the C/O ratio on the gas-phase evolution of C2S and C3S. The simulation results show that the C/O ratio is an important parameter, playing a fundamental role in determining the gas-phase abundances of sulfur species in dense cores.
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页码:134 / 137
页数:4
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