Physical properties and chemical composition of the cores in the California molecular cloud
Physical properties and chemical composition of the cores in the California molecular cloud
复制标题
加州分子云核心的物理性质和化学成分
DOI:
10.1051/0004-6361/201833622
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发表时间:
2018-10
影响因子:
6.5
通讯作者:
Gao Yang
中科院分区:
文献类型:
--
作者:
Zhang Guo-Yin;Xu Jin-Long;Vasyunin A. I.;Semenov D. A.;Wang Jun-Jie;Dib Sami;Liu Tie;Liu Sheng-Yuan;Zhang Chuan-Peng;Liu Xiao-Lan;Wang Ke;Li Di;Wu Zhong-Zu;Yuan Jing-Hua;Li Da-Lei;Gao Yang
Aims. We aim to reveal the physical properties and chemical composition of the cores in the California molecular cloud (CMC), so as to better understand the initial conditions of star formation. Methods. We made a high-resolution column density map (18.2′
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DOI:
10.1088/0004-637x/806/1/31
发表时间:
2015-04
期刊:
The Astrophysical Journal
影响因子:
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作者:
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通讯作者:
M. Gong;E. Ostriker
DOI:
10.1086/166791
发表时间:
1988-10
期刊:
The Astrophysical Journal
影响因子:
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通讯作者:
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DOI:
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发表时间:
1988
期刊:
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影响因子:
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作者:
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通讯作者:
R. Larson
DOI:
10.1086/588608
发表时间:
2008-01
期刊:
The Astrophysical Journal Letters
影响因子:
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作者:
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通讯作者:
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DOI:
10.3847/0004-637x/823/2/160
发表时间:
2016-04
期刊:
The Astrophysical Journal
影响因子:
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作者:
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通讯作者:
M. Dunham;S. Offner;J. Pineda;T. Bourke;J. Tobin;H. Arce;Xuepeng Chen;J. Francesco;D. Johnstone;Katherine I. Lee;P. Myers;D. Price;S. Sadavoy;S. Schnee