Evolution of the spectrum and VLBI structure of W75N during the huge OH maser flare in 2003-2007
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/404/3/1121/18691215/mnras0404-1121.pdf
Reference20 articles.
1. The brightest OH maser in the sky: A flare of emission in W75 N
2. Kinematics of W3(OH) - First proper motions of OH masers from VLBI measurements
3. Interpretation of the VLBI maps of maser spots
4. Full‐Polarization Observations of OH Masers in Massive Star‐forming Regions. II. Maser Properties and the Interpretation of Polarization
5. Large Magnetic Fields and Motions of OH Masers in W75N
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1. Monitoring of the polarized H2O maser emission around the massive protostars W75N(B)-VLA 1 and W75N(B)-VLA 2;Astronomy & Astrophysics;2023-04-24
2. Evolution of OH Maser Emission in the Active Star-Forming Region W75 N. II. Research in the 1667 and 1720 MHz Lines;Astronomy Reports;2022-08
3. 6 cm OH Masers in Northern Star Formation Regions;The Astrophysical Journal;2022-04-01
4. VLBA SURVEYS OF OH MASERS IN STAR-FORMING REGIONS. I. SATELLITE LINES;The Astrophysical Journal;2016-05-11
5. The catalogues and mid-infrared environment of interstellar OH masers;Monthly Notices of the Royal Astronomical Society;2014-05-27
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