A new faint milky way satellite discovered in the Pan-STARRS1 3π Survey

  • Benjamin P.M. Laevens
  • , Nicolas F. Martin
  • , Rodrigo A. Ibata
  • , Hans Walter Rix
  • , Edouard J. Bernard
  • , Eric F. Bell
  • , Branimir Sesar
  • , Annette M.N. Ferguson
  • , Edward F. Schlafly
  • , Colin T. Slater
  • , William S. Burgett
  • , Kenneth C. Chambers
  • , Heather Flewelling
  • , Klaus A. Hodapp
  • , Nicholas Kaiser
  • , Rolf Peter Kudritzki
  • , Robert H. Lupton
  • , Eugene A. Magnier
  • , Nigel Metcalfe
  • , Jeffrey S. Morgan
  • Paul A. Price, John L. Tonry, Richard J. Wainscoat, Christopher Waters

Research output: Contribution to journalArticlepeer-review

152 Scopus citations

Abstract

We present the discovery of a faint Milky Way satellite, Laevens 2/Triangulum II, found in the Panoramic Survey Telescope And Rapid Response System 3π imaging data and confirmed with follow-up wide-field photometry from the Large Binocular Cameras. The stellar system, with an absolute magnitude of MV = -1.8 ± 0.5, a heliocentric distance of 30-2+2 kpc, and a half-mass - radius of 34-8+9 pc, shows remarkable similarity to faint, nearby, small satellites such as Willman 1, Segue 1, Segue 2, and Boötes II. The discovery of Laevens 2/Triangulum II further populates the region of parameter space for which the boundary between dwarf galaxies and globular clusters becomes tenuous. Follow-up spectroscopy will ultimately determine the nature of this new satellite, whose spatial location hints at a possible connection with the complex Triangulum - Andromeda stellar structures.

Original languageEnglish (US)
Article numberL18
JournalAstrophysical Journal Letters
Volume802
Issue number2
DOIs
StatePublished - Apr 1 2015

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: dwarf
  • Galaxy: structure
  • Globular clusters: general
  • Local group

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