Large-Scale Mapping Observations of the C [CSC]i[/CSC] ([TSUP]3[/TSUP][ITAL]P[/ITAL][TINF]1[/TINF]–[TSUP]3[/TSUP][ITAL]P[/ITAL][TINF]0[/TINF]) and CO ([ITAL]J[/ITAL] = 3–2) Lines toward the Orion A Molecular Cloud-Reference-Cited by-同舟云学术

Large-Scale Mapping Observations of the C [CSC]i[/CSC] ([TSUP]3[/TSUP][ITAL]P[/ITAL][TINF]1[/TINF]–[TSUP]3[/TSUP][ITAL]P[/ITAL][TINF]0[/TINF]) and CO ([ITAL]J[/ITAL] = 3–2) Lines toward the Orion A Molecular Cloud

Published:1999-12-10 Issue:1 Volume:527 Page:L59-L62
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Ikeda Masafumi,Maezawa Hiroyuki,Ito Tetsuya,Saito Gaku,Sekimoto Yutaro,Yamamoto Satoshi,Tatematsu Ken’ichi,Arikawa Yuji,Aso Yoshiyuki,Noguchi Takashi,Shi Sheng-Cai,Miyazawa Keisuke,Saito Shuji,Ozeki Hiroyuki,Fujiwara Hideo,Ohishi Masatoshi,Inatani Junji

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. Filamentary structure in the Orion molecular cloud

2. The Orion Molecular Cloud and Star-Forming Region

3. Star formation in the L1641 North cluster

4. (C-12)/(C-13) isotope ratio in the local interstellar medium from observations of (C-13)(O-18) in molecular clouds

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