The molecular core in G34.3 + 0.2 - Millimeter interferometric observations of HCO(+), H(C-13)N, H(C-15)N, and SO-Reference-Cited by-同舟云学术

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The molecular core in G34.3 + 0.2 - Millimeter interferometric observations of HCO(+), H(C-13)N, H(C-15)N, and SO

Published:1992-01 Issue: Volume:385 Page:244
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Carral Patricia,Welch William J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 40 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Excited Hydroxyl Outflow in the High-mass Star-forming Region G34.26 + 0.15;The Astrophysical Journal;2023-08-01

2. Deep, Broadband Spectral Line Surveys of Molecule-rich Interstellar Clouds;The Astrophysical Journal Supplement Series;2017-08-23

3. Water deuterium fractionation in the high-mass hot core G34.26+0.15;Astronomy & Astrophysics;2013-01-23

4. Multiple Outflows Traced by H2O Masers around the Ultra-Compact H II Region G 34.26+0.15;Publications of the Astronomical Society of Japan;2011-12-25

5. Molecular absorption lines toward star-forming regions: a comparative study of HCO+, HNC, HCN, and CN;Astronomy and Astrophysics;2010-09

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