Online Database of Class I Methanol Masers
arXiv:1911.04742 · doi:10.3847/1538-3881/ab4b4c
Abstract
In this paper, we present a database of class I methanol masers. The compiled information from the available literature provides an open and fast access to the data on class I methanol maser emission, including search, analysis and visualization of the extensive maser data set. There is information on individual maser components detected with single-dish observations and maser spots obtained from interferometric data. At the moment the database contains information from ~100 papers, i.e. ~7500 observations and ~650 sites of class I methanol masers. Analysis of the data collected in the database shows that the distribution of class I methanol maser sources is similar to that of class II methanol masers. They are mostly found in the Molecular Ring, where majority of the OB stars are located. The difference between class I and II distributions is the presence of many class I methanol masers in the Nuclear Disk region (Central Molecular Zone). Access to the class I methanol maser database is available online at http://maserdb.net
Accepted to the Astronomical Journal
References in corpus (23)
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Cited by in corpus (13)
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- A Global View on Star Formation: The GLOSTAR Galactic Plane Survey V. 6.7 GHz Methanol Maser Catalogue
- AGB interlopers in YSO catalogues hunted out by NEOWISE
- 44 GHz methanol masers: Observations toward 95 GHz methanol masers
- Variations of the HCO, HCN, HNC, NH and NH deuterium fractionation in high-mass star-forming regions
- Distributions and Physical Properties of Molecular Clouds in the Third Galactic Quadrant: = [219.75, 229.75] and = [-5.25, 5.25]
- The methanol emission in the A line series as a tracer of specific physical conditions in high-mass star-forming regions
- Modelling cosmic masers in C-type shock waves -- the coexistence of Class I CH3OH and 1720 MHz OH masers
- Physical Properties and Kinematics of Dense Cores Associated with Regions of Massive Star Formation from the Southern Sky
- Ammonia mapping observations of the Galactic infrared bubble N49: Three NH clumps along the molecular filament
- Structural and spectral properties of Galactic plane variable radio sources
- Properties of Contracting Massive Protostellar Cores
- Modelling carbon chain and complex organic molecules in the DR21(OH) clump