Abstract
We report the discovery of a significant and compact over-density of old and metal-poor stars in the fourth data release of the KiDS survey (DR4). The discovery is confirmed by deeper HSC-SSP data revealing the old main sequence turn-off of a stellar system located at a distance from the sun of D = 145-13+14 kpc in the direction of the Sextans constellation. The system has an absolute integrated magnitude (MV = -3.9 ± 0.4), half-light radius (rh = 193-46+61 pc), and ellipticity (e = 0.46-0.15+0.11) values that are typical of ultra-faint dwarf galaxies (UFDs). The central surface brightness is near the lower limits of known local dwarf galaxies of a similar integrated luminosity, as expected for stellar systems that have escaped detection until now. The distance of the newly found system suggests that it is likely to be a satellite of our own Milky Way and we have thus tentatively named it Sextans II (KiDS-UFD-1).
Original language | English |
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Article number | L13 |
Number of pages | 7 |
Journal | Astronomy and Astrophysics |
Volume | 681 |
DOIs | |
Publication status | Published - 1-Jan-2024 |
Keywords
- Galaxies: clusters: general
- Galaxies: dwarf
- Galaxies: photometry
- Galaxy: halo
- Hertzsprung-Russell and C-M diagrams
- Surveys