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The Southern HII Region Discovery Survey. II. The Full Catalog

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arxiv 2103.12199 v1 pith:7SNBR6EY submitted 2021-03-22 astro-ph.GA

The Southern HII Region Discovery Survey. II. The Full Catalog

classification astro-ph.GA
keywords regionregionsgalacticcandidatescontinuumknownpreviouslycatalog
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Southern HII Region Discovery Survey (SHRDS) is a 900 hour Australia Telescope Compact Array 4-10 GHz radio continuum and radio recombination line (RRL) survey of Galactic HII regions and infrared-identified HII region candidates in the southern sky. For this data release, we reprocess all previously published SHRDS data and include an additional ~450 hours of observations. The search for new HII regions is now complete over the range 259 deg < Galactic longitude < 346 deg, |Galactic latitude| < 4 deg for HII region candidates with predicted 6 GHz continuum peak brightnesses >30 mJy/beam. We detect radio continuum emission toward 730 targets altogether including previously known nebulae and HII region candidates. By averaging ~18 RRL transitions, we detect RRL emission toward 206 previously known HII regions and 436 HII region candidates. Including the northern sky surveys, over the last decade the HII Region Discovery Surveys have more than doubled the number of known Galactic HII regions. The census of HII regions in the WISE Catalog of Galactic HII Regions is now complete for nebulae with 9 GHz continuum flux densities > 250 mJy. We compare the RRL properties of the newly discovered SHRDS nebulae with those of all previously known HII regions. The median RRL full-width at half-maximum line width of the entire WISE Catalog HII region population is 23.9 km/s and is consistent between Galactic quadrants. The observed Galactic longitude-velocity asymmetry in the population of HII regions probably reflects underlying spiral structure in the Milky Way.

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Cited by 1 Pith paper

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    Forward modeling of multi-frequency HRRLs at 342 MHz, 800 MHz and 5.8 GHz constrains electron densities of dense warm ionized gas in the Galactic plane to 6–15 cm^{-3}.