New KiDS in town: Sextans II: A new stellar system on the outskirts of the Milky Way

Massimiliano Gatto, Michele Bellazzini, Crescenzo Tortora, Vincenzo Ripepi, Massimo Dall'ora, Michele Cignoni, Konrad Kuijken, Hendrik Hildebrandt, Shiyang Zhang, Jelte De Jong, Nicola R. Napolitano, Simon E.T. Smith

Research output: Contribution to journalArticleAcademicpeer-review

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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 languageEnglish
Article numberL13
Number of pages7
JournalAstronomy and Astrophysics
Volume681
DOIs
Publication statusPublished - 1-Jan-2024

Keywords

  • Galaxies: clusters: general
  • Galaxies: dwarf
  • Galaxies: photometry
  • Galaxy: halo
  • Hertzsprung-Russell and C-M diagrams
  • Surveys

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