M
Maxim Voronkov
Researcher at Commonwealth Scientific and Industrial Research Organisation
Publications - 142
Citations - 6826
Maxim Voronkov is an academic researcher from Commonwealth Scientific and Industrial Research Organisation. The author has contributed to research in topics: Maser & Galaxy. The author has an hindex of 40, co-authored 139 publications receiving 6036 citations. Previous affiliations of Maxim Voronkov include Australia Telescope National Facility.
Papers
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Journal ArticleDOI
The methanol multibeam survey
James Green,R. J. Cohen,J. L. Caswell,Gary A. Fuller,Kate J. Brooks,Michael G. Burton,Antonio Chrysostomou,Philip J. Diamond,Simon Ellingsen,Malcolm Gray,Melvin Hoare,M. R. W. Masheder,Naomi McClure-Griffiths,M. R. Pestalozzi,Chris Phillips,L. Quinn,Mark Thompson,Maxim Voronkov,Andrew Walsh,Derek Ward-Thompson,D. Wong-McSweeney,Jeremy Yates,J. Cox +22 more
TL;DR: The Methanol Multibeam (MMB) survey as mentioned in this paper was used to survey the Galactic plane for newly forming high mass stars, pinpointed by strong methanol maser emission at 6.7 GHz.
Posted Content
Molecular line search toward the flaring 6.7-GHz methanol masers of G24.33+0.13 and G359.6-0.243: rare maser transitions detected
T. P. McCarthy,Gabor Orosz,Simon Ellingsen,Shari Breen,Maxim Voronkov,Ross A. Burns,M. Olech,Yoshinori Yonekura,Tomoya Hirota,Lucas J. Hyland,Paweł Wolak +10 more
TL;DR: In this paper, the authors performed a molecular line search toward the flaring 6.7-GHz masers G24.33+0.13 and G359.62-0.24 using the Australia Telescope Compact Array.
Journal ArticleDOI
What is happening in G357.96-0.16?
TL;DR: In this article, the relationship between two sites of maser activity in G357.96-0.16 is examined, and future observations for examining the dust properties of this interesting region of massive star formation are proposed.
Journal ArticleDOI
High-velocity feature of the class I methanol maser in G309.38-0.13
Maxim Voronkov,James Caswell,T. R. Britton,T. R. Britton,J. A. Green,A. M. Sobolev,Simon Ellingsen +6 more
TL;DR: In this paper, the Australia Telescope Compact Array (ATCA) has been used to map class I methanol masers at 36 and 44 GHz in G309.38-0.13 GHz, and the data allowed the discovery of a high-velocity 36-GHz spectral feature, which is blue-shifted by about 30 km/s from the peak velocity at this frequency, but spatially located close to (within a few arcseconds of) the brightest maser spot.
Journal ArticleDOI
Maser action in methanol transitions
TL;DR: In this paper, the ATCA was used to detect 6.7 GHz methanol emission towards OMC-1. The source has a size between 40'' and 90'' and is located to the south-east of Ori-KL and may coincide in position with the 25 GHz masers.