Discovery of periodic methanol masers associated with G323.46−0.08

Author:

Proven-Adzri E12ORCID,MacLeod G C34,Heever S P van den4,Hoare M G5,Kuditcher A1,Goedhart S6ORCID

Affiliation:

1. Department of Physics, University of Ghana, P. O. Box LG 63, Legon, Accra, Ghana

2. Ghana Space Science and Technology Institute, Ghana Atomic Energy Commission, P.O. Box LG 80, Legon, Accra, Ghana

3. The University of Western Ontario, 1151 Richmond Street, London, ON N6A 3K7, Canada

4. Hartebeesthoek Radio Astronomy Observatory, PO Box 443, Krugersdorp, 1741, South Africa

5. School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK

6. SARAO, 2 Fir Street, Black River Park, Observatory 7925, Cape Town, South Africa

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 14 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. Seven-year periodic variations in the methanol maser line displayed by the massive protostar IRAS 20216+4104;Astronomy & Astrophysics;2024-01-29

2. Detection of the longest periodic variability in 6.7 GHz methanol masers of G5.900−0.430;Publications of the Astronomical Society of Japan;2023-01-27

3. Episodic accretion and mergers during growth of massive protostars;Monthly Notices of the Royal Astronomical Society;2022-10-28

4. The burst mode of accretion in massive star formation with stellar inertia;Monthly Notices of the Royal Astronomical Society;2022-10-16

5. Millimeter methanol emission in the high-mass young stellar object G24.33+0.14;Publications of the Astronomical Society of Japan;2022-09-05

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