Far‐Infrared Spectroscopy of C ii and High‐ J CO Emission from Warm Molecular Gas in NGC 3576-Reference-Cited by-同舟云学术

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Far‐Infrared Spectroscopy of C ii and High‐ J CO Emission from Warm Molecular Gas in NGC 3576

Published:1997-08 Issue:2 Volume:111 Page:409-417
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:en
Short-container-title:ASTROPHYS J SUPPL S

Author:

Boreiko R. T.,Betz A. L.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference37 articles.

1. H66 radio recombination line observations of southern H II regions

2. Observations of the J = 1-0 transition of HCO+ in southern molecular clouds

3. Betz, A. L. & Boreiko, R. T. 1993, in ASP Conf. Proc. 41, Astronomical Infrared Spectroscopy, ed. S. Kwok (San Francisco: ASP), 349

4. Heterodyne spectroscopy of the J = 17-16 CO line in Orion

5. Line emission from clumpy photodissociation regions

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1. Synthetic [C ii] emission maps of a simulated molecular cloud in formation;Monthly Notices of the Royal Astronomical Society;2018-09-18

2. HERSCHELEXTREME LENSING LINE OBSERVATIONS: [C ii] VARIATIONS IN GALAXIES AT REDSHIFTSz= 1–3;The Astrophysical Journal;2017-01-20

3. EVOLUTION OF MASS OUTFLOW IN PROTOSTARS;The Astrophysical Journal;2016-08-29

4. OBSERVATIONS OF WARM CARBON CHAIN CHEMISTRY IN NGC 3576;The Astrophysical Journal;2014-12-18

5. Opportunities for Terahertz Facilities on the High Plateau;Proceedings of the International Astronomical Union;2012-08

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