KK 242, a faint companion to the isolated Scd galaxy NGC 6503
arXiv:2111.14691 · doi:10.3847/1538-3881/ac3cbe
Abstract
Using Hubble Space Telescope imaging of the resolved stellar population of KK~242 = NGC6503-d1 = PGC~4689184, we measure the distance to the galaxy to be Mpc and find that KK~242 is a satellite of the low-mass spiral galaxy NGC~6503 located on the edge of the Local Void. Observations with the Karl G. Jansky Very Large Array show signs of a very faint HI-signal at the position of KK~242 within a velocity range of km\,s. This velocity range is severely contaminated by HI emission from the Milky Way and from NGC6503. The dwarf galaxy is classified as the transition type, dIrr/dSph, with a total HI-mass of and a star formation rate SFR(H) = --4.82 dex (/yr). Being at a projected separation of 31 kpc with a radial velocity difference of -- 105 km\,s relative to NGC~6503, KK~242 gives an estimate of the halo mass of the spiral galaxy to be ) = 11.6. Besides NGC~6503, there are 8 more detached low-luminosity spiral galaxies in the Local Volume: M~33, NGC~2403, NGC~7793, NGC~1313, NGC~4236, NGC~5068, NGC~4656 and NGC~7640, from whose small satellites we have estimated the average total mass of the host galaxies and their average total mass-to-K-band-luminosity and , respectively.
Accepted for publication in the Astronomical Journal
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