2002MNRAS.333..871J

Query : 2002MNRAS.333..871J

2002MNRAS.333..871J - Mon. Not. R. Astron. Soc., 333, 871-875 (2002/July-2)

A probable planetary companion to HD 39091 from the Anglo-Australian Planet Search.

JONES H.R.A., BUTLER R.P., TINNEY C.G., MARCY G.W., PENNY A.J., McCARTHY C., CARTER B.D. and POURBAIX D.

Abstract (from CDS):

We report the detection of an extra-solar planet candidate orbiting the G1 V star HD 39091. The orbital period is 2049d and the eccentricity is 0.62. With a minimum (M sini) mass of 10.3MJUP this object falls near the high-mass end of the observed planet mass function, and may plausibly be a brown dwarf. Other characteristics of this system, including orbital eccentricity and metallicity, are typical of the well-populated class of radial velocity planets in eccentric orbits around metal-rich stars.

Abstract Copyright: 2002 Blackwell Science Ltd

Journal keyword(s): stars: individual: HD 39091 - stars: low-mass, brown dwarfs - planetary systems

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * pi. Men b Pl 05 37 09.8868446714 -80 28 08.834553264           ~ 82 1
2 * pi. Men PM* 05 37 09.8868446714 -80 28 08.834553264   6.25 5.67     G0V 390 1

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