Aldebaran b's Temperate Past Uncovered in Planet Search Data

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DOI

    Will M. Farr, Flatiron Inst, Ctr Computat Astrophys, Benjamin J. S. Pope, NYU, New York University, Dept Phys, Ctr Cosmol & Particle Phys, Guy R. Davies, Univ Birmingham, University of Birmingham, Sch Phys & Astron, Thomas S. H. North, Univ Birmingham, University of Birmingham, Sch Phys & Astron, Timothy R. White, Jim W. Barrett, Univ Birmingham, University of Birmingham, Sch Phys & Astron,
  • Andrea Miglio
  • Mikkel N. Lund
  • Victoria Antoci
  • Mads Fredslund Andersen
  • Frank Grundahl
  • Daniel Huber, Univ Sydney, University of Sydney, Sydney Inst Astron SIfA, Sch Phys, Univ Hawaii, University of Hawaii System, Inst Astron, SETI Inst
Original languageEnglish
Article number20
JournalAstrophysical Journal Letters
Volume865
Issue number2
Number of pages12
ISSN2041-8205
DOIs
Publication statusPublished - 1 Oct 2018

    Research areas

  • methods: data analysis, methods: statistical, planets and satellites: individual (Aldebaran b), stars: individual (Aldebaran), stars: oscillations (including pulsations), techniques: radial velocities, RADIAL-VELOCITY VARIATIONS, LONG SECONDARY PERIODS, RED GIANTS, SPACED DATA, STARS, DIAMETER, LINE, ASTEROSEISMOLOGY, CONFIRMATION, VARIABILITY

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