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On the Relationship of UC H II Regions and Class II Methanol Masers: I. Source Catalogs

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arxiv 1609.03280 v1 pith:RHEL5G5W submitted 2016-09-12 astro-ph.GA

On the Relationship of UC H II Regions and Class II Methanol Masers: I. Source Catalogs

classification astro-ph.GA
keywords masersmasermethanolsourcescatalogscontinuumassociatedclass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We conducted VLA C-configuration observations to measure positions and luminosities of Galactic Class II 6.7 GHz methanol masers and their associated ultra-compact H II regions. The spectral resolution was 3.90625 kHz and the continuum sensitivity reached 45 \uJypb. We mapped 372 methanol masers with peak flux densities of more than 2 Jy selected from the literature, 367 of them were detected. Absolute positions have nominal uncertainties of 0.3 arcsec. In this first paper on the data analysis, we present three catalogs, the first gives information on the strongest feature of 367 methanol maser sources, and the second on all detected maser spots. The third catalog present derived data of the 279 radio continuum sources found in the vicinity of maser sources. Among them, 140 show evidence of physical association with maser sources. Our catalogs list properties including distance, flux density, radial velocity and the distribution of masers on the Galactic plane is then provided as well. We found no significant relationship between luminosities of masers and their associated radio continuum counterparts.

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Cited by 2 Pith papers

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    Polarization observations of 6.7 GHz methanol masers show linear and circular components with Zeeman splitting that varies over time, interpreted as evidence for changing magnetic fields.

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    Maser emissions act as cosmic rulers for astrometric measurements of astronomical sources from protostellar scales to galactic distances, with SKA-Mid enabling expanded multi-species observations.