Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey
arXiv:2409.16607 · doi:10.1051/0004-6361/202451038
Abstract
Context. Sensitive radio continuum data could remove the difference between the number of known supernova remnants (SNRs) in the Galaxy compared to that expected, but due to confusion in the Galactic plane, faint SNRs can be challenging to distinguish from brighter HII regions and filamentary radio emission. Aims. We wish to exploit new SARAO MeerKAT 1.3 GHz Galactic Plane Survey (SMGPS) radio continuum data, which covers and at , to search for SNR candidates in the Milky Way disk. Methods. We also use MIR data from the Spitzer GLIMPSE, Spitzer MIPSGAL, and WISE surveys to help identify SNR candidates. The identified SNR candidate are sources of extended radio continuum emission that lack MIR counterparts, are not known as HII regions in the WISE Catalog of Galactic HII Regions, and are not known previously as SNRs Results. We locate 237 new Galactic SNR candidates in the SMGPS data. We also identify and confirm the expected radio morphology for 201 objects listed in the literature as being SNRs and 130 previously-identified SNR candidates. The known and candidate SNRs have similar spatial distributions and angular sizes. Conclusions. The SMGPS data allowed us to identify a large population of SNR candidates that can be confirmed as true SNRs using radio polarization measurements or by deriving radio spectral indices. If the 237 candidates are confirmed as true SNRs, it would approximately double the number of known Galactic SNRs in the survey area, alleviating much of the difference between the known and expected populations.
Accepted by A&A. Images and FITS files of each source can be found here: https://doi.org/10.48479/0n8c-5q84
References in corpus (13)
- The VLA Galactic Plane Survey
- Discovery of 35 New Supernova Remnants in the Inner Galaxy
- Dependence of Interstellar Turbulent Pressure on Supernova Rate
- The 1.28 GHz MeerKAT DEEP2 Image
- Galactic Supernova Remnant Candidates Discovered by THOR
- A global view on star formation: The GLOSTAR Galactic Plane Survey. I. Overview and first results for the Galactic longitude range 28° < l < 36°
- The Expansion and Radio Spectral Index of G21.5-0.9: Is PSR J1833-1034 the Youngest Pulsar?
- Distances, Radial Distribution and Total Number of Galactic Supernova Remnants
- A global view on star formation: The GLOSTAR Galactic plane survey. II. Supernova Remnants in the first quadrant of the Milky Way
- Candidate radio supernova remnants observed by the GLEAM survey over and
- A Catalogue of Radio Supernova Remnants and Candidate Supernova Remnants in the EMU/POSSUM Galactic Pilot Field
- The variability of the Crab Nebula in radio: No radio counterpart to gamma-ray flares
- Radio Observations of the Region around the Pulsar Wind Nebula HESS J1303-631 with ATCA
Cited by in corpus (9)
- A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I
- The SARAO MeerKAT Galactic Plane Survey extended source catalogue
- GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended (GLEAM-X) III: Galactic Plane
- The infrared counterpart and proper motion of magnetar SGR0501+4516
- MeerKAT discovery of 164 compact radio rings toward the Galactic Plane
- Radio detection of supernova remnant G310.7-5.4 with -ray counterpart: Abeona SNR
- Heavy interstellar scattering toward the near end of the Galactic bar
- A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release
- A newly born spider system at the core of a radio shell: Evidence for a low-energy supernova