University of Hertfordshire

From the same journal

From the same journal

Wide cool and ultracool companions to nearby stars from pan-STARRS 1

Research output: Contribution to journalArticle

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  • 1407.2938v3

    Accepted author manuscript, 2.76 MB, PDF document

  • Niall R. Deacon
  • Michael C. Liu
  • Eugene A. Magnier
  • Kimberly M. Aller
  • William M J Best
  • Trent Dupuy
  • Brendan P. Bowler
  • Andrew W. Mann
  • Joshua A. Redstone
  • William S. Burgett
  • Kenneth C. Chambers
  • Peter W. Draper
  • H. Flewelling
  • Klaus W. Hodapp
  • Nick Kaiser
  • Rolf Peter Kudritzki
  • Jeff S. Morgan
  • Nigel Metcalfe
  • Paul A. Price
  • John L. Tonry
  • And 1 others
  • Richard J. Wainscoat
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Original languageEnglish
Article number119
Number of pages40
JournalThe Astrophysical Journal
Volume792
Issue2
DOIs
Publication statusPublished - 22 Aug 2014

Abstract

We present the discovery of 57 wide (>5″) separation, low-mass (stellar and substellar) companions to stars in the solar neighborhood identified from Pan-STARRS 1 (PS1) data and the spectral classification of 31 previously known companions. Our companions represent a selective subsample of promising candidates and span a range in spectral type of K7-L9 with the addition of one DA white dwarf. These were identified primarily from a dedicated common proper motion search around nearby stars, along with a few as serendipitous discoveries from our Pan-STARRS 1 brown dwarf search. Our discoveries include 23 new L dwarf companions and one known L dwarf not previously identified as a companion. The primary stars around which we searched for companions come from a list of bright stars with well-measured parallaxes and large proper motions from the Hipparcos catalog (8583 stars, mostly A-K dwarfs) and fainter stars from other proper motion catalogs (79170 stars, mostly M dwarfs). We examine the likelihood that our companions are chance alignments between unrelated stars and conclude that this is unlikely for the majority of the objects that we have followed-up spectroscopically. We also examine the entire population of ultracool (>M7) dwarf companions and conclude that while some are loosely bound, most are unlikely to be disrupted over the course of ∼10 Gyr. Our search increases the number of ultracool M dwarf companions wider than 300 AU by 88% and increases the number of L dwarf companions in the same separation range by 82%. Finally, we resolve our new L dwarf companion to HIP 6407 into a tight (0.″13, 7.4 AU) L1+T3 binary, making the system a hierarchical triple. Our search for these key benchmarks against which brown dwarf and exoplanet atmosphere models are tested has yielded the largest number of discoveries to date.

Notes

© 2014. The American Astronomical Society. All rights reserved.

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