The Southern HII Region Discovery Survey. II. The Full Catalog
arXiv:2103.12199 · doi:10.3847/1538-4365/abf4d4
Abstract
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.
37 pages, 10 figures, 11 tables (full tables in machine readable format available in the online journal), 1 appendix. Survey website: https://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/en/community/shrds/
References in corpus (12)
- The NumPy array: a structure for efficient numerical computation
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
- Radio Recombination Lines in Galactic HII Regions
- Metallicity Structure in the Milky Way Disk Revealed by Galactic HII Regions
- Survey of Ionized Gas of the Galaxy, Made with the Arecibo telescope (SIGGMA): Inner Galaxy Data Release
- The Southern HII Region Discovery Survey I: The Bright Catalog
- The Southern HII Region Discovery Survey (SHRDS): Pilot Survey
- A 4-6 GHz Radio Recombination Line Survey in the Milky Way
- The Galactic HII Region Luminosity Function at Radio and Infrared Wavelengths
- Re-analysis of the radio luminosity function of Galactic HII regions
- A VLA Census of the Galactic H II Region Population
Cited by in corpus (8)
- The detection of a hot molecular core in the extreme outer Galaxy
- Peering into the Milky Way by FAST: II. Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
- SPLASH: The Southern Parkes Large-Area Survey in Hydroxyl -- Data Description & Release
- A global view on star formation: The GLOSTAR Galactic plane survey X. Galactic HII region catalog using radio recombination lines
- Parallax-based Distances to Galactic Hii Regions: Nearby Spiral Structure
- New Massive Contact Twin Binary in a Radio-quiet HII Region Associated with the M17 Complex
- Discovery of a New Population of Galactic HII Regions with Ionized Gas Velocity Gradients
- Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations