A sensitive search for water masers associated with star formation regions in the Local Group galaxy NGC 6822
arXiv:2205.00545 · doi:10.1017/pasa.2022.8
Abstract
We report the results of a sensitive search for water maser emission in the Local Group Galaxy NGC 6822 with the Karl G. Jansky Very Large Array. The observations provide tentative single-epoch detections of four candidates, associated with two infrared-bright star formation regions (Hubble I/III and Hubble IV). The candidate maser detections are all offset from the velocity range where strong emission from HI neutral gas is observed toward NGC 6822, with the closest offset by 40 kms. Our observations include the location of NL1K, a previous tentative water maser detection in NGC 6822. We do not detect any emission from this location with a sensitivity limit approximately a factor of 5 better than the original Sardina Radio Telescope observations.
Accepted for publication by the Publications of the Astronomical Society of Australia: 8 pages, 7 figures
References in corpus (9)
- Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way
- Accurate water maser positions from HOPS
- Water maser variability over 20 years in a large sample of star-forming regions: the complete database
- The Proper Motion of the Local Group Galaxy IC 10
- The Nature of Infrared Emission in the Local Group Dwarf Galaxy NGC 6822 As Revealed by Spitzer
- Solo dwarfs III: Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
- Water masers in the Local Group of galaxies
- HI Kinematics, Mass Distribution, and Star Formation Threshold in NGC 6822, using the SKA pathfinder KAT-7
- Sardinia Radio Telescope observations of Local Group dwarf galaxies -- I. The cases of NGC6822, IC1613, and WLM