From the Extrasolar Planets Encyclopaedia : http://exoplanet.eu 
Planet : VB 10 b
THE PLANET
Basic data : 
 
Name VB 10 b
Discovered in2009   
M.sin i6.4 (−3.1+2.6MJ ref.
Semi major axis0.36 (−0.006+0.016AU ref.
Orbital period271.56 (−3+6.9days ref.
Eccentricity< 0.98   ref.
ω38.7 (−3.3+4.8deg. ref.
Inclination96.9 (−1.8+7.4deg. ref.
Update18/12/09   
No molecule detected
 
Remarks : 
 2 Dec. 2009: Planet VB 10 b not seen in CRIRES radial velocity data (Baen et al. 2009)
 11 related publications :  (sort by author)  (sort by date)
 
 
HARRINGTON R., KALLARAKAL V. & DAHN C. , 1983
Astrometry of the low-luminosity stars VB8 and VB10
Astron. J. , 88 , 1038
abstarct
 
 
PRAVDO S. & SHAKLAN S. , 2009
An ultracool star's candidate planet
ApJ. , 700 , 623
paper
 
 
MONET D., DAHN C., VRBA F., HARRIS H., PIER J., LUGINBUHL Ch. & ABLES A. , 2009
U.S. Naval Observatory CCD parallaxes of faint stars. I - Program description and first results
Astron. J. , 103 , 638
 
 
ZAPATERO-OSORIO M.-R., MARTIN E., del BURGO C., DESHPANDE R., RODIER F. & MONTGOMERY M. , 2009
Infrared radial velocities of vB 10
Astron. & Astrophys. , 505 , L5
paper
 
 
CAMPANELLA G. , 2009
The search for exomoons and the characterization of exoplanet atmospheres
Roma, MSc Thesis, 4 September 2009
Full text
 
 
BEAN J., SEIFAHRT A., HARTMAN H., NILSSON H., REINERS A., DREIZLER S., HENRY T. & WIEDEMANN G , 2009
The Proposed Giant Planet Orbiting VB 10 Does Not Exist
ApJ. Letters , 711 , L19
paper
 
 
ANGLADA-ESCUDE G., SHKOLNIK E., WEINBERGER A., THOMPSON I. & OSIP D. , 2010
Strong Constraints to the Putative Planet Candidate around VB 10 using Doppler spectroscopy
ApJ. Letters , 711 , L24
paper
 
 
WRIGHT J., MARCY G. & the California Planet Survey consortium , 2010
Exoplanet Data Explorer
web page
 
 
POPPENHAEGER K., ROBRADE J. & SCHMITT J. , 2010
Coronal properties of planet-bearing stars
Astron. & Astrophys. , - , -
accepted
preprint
 
 
BEAN J., SEIFAHRT A., HARTMAN H., NILSSON H., WIEDEMANN G., REINERS A., DREIZLER S. & HENRY T. , 2010
The CRIRES Search for Planets at the Bottom of the Main Sequence
The Mesenger , no 140 , 41
paper
 
 
DONNISON J. , 2010
The Hill stability of the possible moons of extrasolar planets
MNRAS , 406 , 1918
paper
THE STAR
Basic data :   
More data : 
  - Basic data (from Simbad)
- Most recent ref (from ADS)
 
Name VB 10
Distance5.83 (± 0.05) pc ref.
Spectral TypeM8V   
Apparent Magnitude V17.3   
Apparent Magnitude H9.23   
Apparent Magnitude J9.91   
Apparent Magnitude K8.77   
Mass0.0779 Msun ref.
Right Asc. Coord.19 16 58   
Decl. Coord.+05 09 02