44 GHz Class I Methanol (CHOH) Maser Survey in the Galactic Center
arXiv:1606.02257 · doi:10.3847/0004-637X/832/2/129
Abstract
We report on a large 44 GHz ( A) methanol (CHOH) maser survey of the Galactic Center (GC). The Karl G. Jansky Very Large Array was used to search for CHOH maser emission covering a large fraction of the region around Sgr A. In 25 pointings, over 300 CHOH maser sources () were detected. The majority of the maser sources have a single peak emission spectrum with line of sight velocities that range from about 13 km\,s to 72 km\,s. Most maser sources were found to have velocities around 3555 km\,s, closely following velocities of neighboring interacting molecular clouds. The full width half maximum of each individual spectral feature is very narrow (0.85 km\,s on average). In the north, where Sgr A East is known to be interacting with the 50 km\,s molecular cloud, more than 100 44 GHz CHOH masers were detected. In addition, three other distinct concentrations of masers were found, which appear to be located closer to the interior of the interacting molecular clouds. Possibly a subset of masers are associated with star formation, although conclusive evidence is lacking.
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Cited by in corpus (7)
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- Diagnostics of a Nuclear Starburst: Water and Methanol Masers
- Molecular Cloud Cores in the Galactic Center 50 Molecular Cloud
- Modelling cosmic masers in C-type shock waves -- the coexistence of Class I CH3OH and 1720 MHz OH masers
- Hot Molecular Core Candidates in the Galactic Center 50 km/s Molecular Cloud
- Parsec-scale SiO emission in the Galactic Center