Revealing the Galactic HiiRegion G84.9+0.5 through 5 GHz Continuum and Polarization Emission and a Voigt Profile Analysis of Radio Recombination Line Observations-Reference-Cited by-同舟云学术

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Revealing the Galactic HiiRegion G84.9+0.5 through 5 GHz Continuum and Polarization Emission and a Voigt Profile Analysis of Radio Recombination Line Observations

Published:2007-09-20 Issue:1 Volume:667 Page:248-256
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Foster T. J.,Kothes R.,Kerton C. R.,Arvidsson K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference44 articles.

1. On the Interpretation of Radio Recombination Line Observations

2. Discovery of 35 New Supernova Remnants in the Inner Galaxy

3. ASpitzer Space TelescopeInfrared Spectrograph Spectral Atlas of Luminous 8 μm Sources in the Large Magellanic Cloud

4. The High‐Resolution IRAS Galaxy Atlas

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1. The Age Evolution of the Radio Morphology of Supernova Remnants;The Astrophysical Journal;2019-10-16

2. Gas kinematics in the H ii regions G351.69-1.15 and G351.63-1.25;Monthly Notices of the Royal Astronomical Society;2016-11-22

3. THE SLOW IONIZED WIND AND ROTATING DISKLIKE SYSTEM THAT ARE ASSOCIATED WITH THE HIGH-MASS YOUNG STELLAR OBJECT G345.4938+01.4677;The Astrophysical Journal;2014-11-13

4. SRAO CO Observation of Supernova Remnants in l = 70° to 190°;Proceedings of the International Astronomical Union;2013-01

5. SRAO CO observation of 11 supernova remnants in l=70∘ to 190∘;Astrophysics and Space Science;2012-08-15

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