4.7 Article

THE CALIFORNIA PLANET SURVEY IV: A PLANET ORBITING THE GIANT STAR HD 145934 AND UPDATES TO SEVEN SYSTEMS WITH LONG-PERIOD PLANETS

Journal

ASTROPHYSICAL JOURNAL
Volume 800, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/800/1/22

Keywords

planetary systems; stars: individual (HD 145934, GJ 849); techniques: radial velocities

Funding

  1. NASA Keck PI Data Awards [2007B_N095Hr, 2010A_N147Hr, 2011AB_N141Hr, 2012A_N129Hr]
  2. NASA Origins of Solar Systems grant [NNX09AB35G]
  3. NASA Astrobiology Institute grant [NNA09DA76A]
  4. Center for Exoplanets and Habitable Worlds (Pennsylvania State University)
  5. Center for Exoplanets and Habitable Worlds (Eberly College of Science)
  6. Center for Exoplanets and Habitable Worlds (Pennsylvania Space Grant Consortium)
  7. NSF [AST-1211441]
  8. NASA [120906, NNX09AB35G] Funding Source: Federal RePORTER
  9. Direct For Mathematical & Physical Scien
  10. Division Of Astronomical Sciences [1211441] Funding Source: National Science Foundation

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We present an update to seven stars with long-period planets or planetary candidates using new and archival radial velocities from Keck-HIRES and literature velocities from other telescopes. Our updated analysis better constrains orbital parameters for these planets, four of which are known multi-planet systems. HD 24040 b and HD 183263 c are super-Jupiters with circular orbits and periods longer than 8 yr. We present a previously unseen linear trend in the residuals of HD 66428 indicative of an additional planetary companion. We confirm that GJ 849 is a multi-planet system and find a good orbital solution for the c component: it is a 1 M-Jup planet in a 15 yr orbit (the longest known for a planet orbiting an M dwarf). We update the HD 74156 double-planet system. We also announce the detection of HD 145934 b, a 2 M-Jup planet in a 7.5 yr orbit around a giant star. Two of our stars, HD 187123 and HD 217107, at present host the only known examples of systems comprising a hot Jupiter and a planet with a well constrained period greater than 5 yr, and with no evidence of giant planets in between. Our enlargement and improvement of long-period planet parameters will aid future analysis of origins, diversity, and evolution of planetary systems.

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