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

4 Citations (Scopus)
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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 & 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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