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Sub-arcsecond (Sub)millimeter Imaging of the Massive Protocluster G358.93−0.03: Discovery of 14 New Methanol Maser Lines Associated with a Hot Core

Journal: The Astrophysical Journal Letters

Published: 2019-08-20

DOI: 10.3847/2041-8213/ab2f8a

Affiliations: 27

Authors: 28

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Institutions Share
NSF National Radio Astronomy Observatory (NRAO), United States of America (USA) 0.14
Harvard-Smithsonian Center for Astrophysics (CfA), United States of America (USA) 0.09
Max Planck Institute for Radio Astronomy (MPIFR), Germany 0.09
Korea Astronomy and Space Science Institute (KASI), South Korea 0.05
Crimean Astrophysical Observatory (CrAO), Ukraine 0.05
Centre for Space Research, NWU, South Africa 0.05
Max Planck Institute for Astronomy (MPIA), Germany 0.04
Mizusawa VLBI Observatory, NAOJ, Japan 0.04
School of Physics and Astronomy, University of St Andrews, United Kingdom (UK) 0.04
Dublin Institute for Advanced Studies (DIAS), Ireland 0.04
Center for Astrophysics, GU, China 0.04
INAF - Astronomical Observatory of Cagliari (OAC), Italy 0.04
National Astronomical Observatory of Japan (NAOJ), NINS, Japan 0.04
Institute of Astronomy and Astrophysics (ASIAA), Academia Sinica, Taiwan 0.04
Karl Schwarzschild Observatory (TLS), Germany 0.04
Ural Federal University (UrFU), Russia 0.04
INAF - Institute of Radioastronomy (IRA), Italy 0.02
Hartebeesthoek Radio Astronomy Observatory (HartRAO), South Africa 0.02
Department of Astronomical Science, Sokendai, Japan 0.02
National Astronomical Research Institute of Thailand, Thailand 0.02
Western University (UWO), Canada 0.02
Italian ALMA Regional Centre (Italian ARC), Italy 0.02
Department of Astronomy, UVA, United States of America (USA) 0.02
Institute of Applied Astronomy (IAA), RAS, Russia 0.02
Department of Physics and Astronomy, UNN, Nigeria 0.01
Department of Physics, NWU, South Africa 0.01

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