What we have found to date:

• Astrometric binaries
  • Barnard's star planets (photographic, HST)
  • Proxima Centauri (fritz benedict (UT) HST results)
  • LHS 1047, LHS 1070, Gl105, et al.

• Pulsar planets
  
  • PSR 1257+12 (Alexander Wolszczan, Penn State)
    3 objects, masses > 0.015 E, 3.4 E, and 2.8 E
  • PSR B0329+54 (Tatiana Shabanova, Lebedev Physical Inst, Moscow)
    18 milliseconds, P ~ 17 yrs, mass > 2 E, a > 7.3 au

• Field BD's
  • GD 165B
  • all very cool M dwarfs?
  • Gl 229 - best case yet
    • AO coronograph detection
    • v.v.red companion 7 arcsec from M primary
    • spectrum shows methane and water [fig]
    • T < 1000 deg K, mass ~ 0.04 - 0.055 S
  • 296A (Jones, Thakerah, Hawkins), dwarf with Li

• Cluster BD's (age is known)
  • PPL 15 (John Stauffer, SAO) Li detected [fig]
  • Teide 1 (Rafaelo Rebolo, Canary Is) Li detected

• Stellar disks
  Vega, Beta Pictoris

• Velocity meter results
  • 51 Pegasi
    Michel Mayor and Didier Queloz (Geneva) - amp ~51 m/s
    Geoff Marcy and Paul Butler (SFSU) confirmation
    P = 4.229+/-0.001 d, e = 0.01 +/- 0.01, mass > 0.46 +/- 0.01 J
    (but David Gray.. ..)
  • 70 Virginis
    Marcy and Butler - amplitude 11 m/s
    P = 3.02 yrs, e ~ 0, mass > 2.3 J
  • 47 Ursa Majoris Marcy and Butler P = 116 d, e = 0.38, mass > 6.5 J
  • and more.. . .

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