2002ApJ...568..369N

Query : 2002ApJ...568..369N

2002ApJ...568..369N - Astrophys. J., 568, 369-376 (2002/March-3)

Determination of masses and other properties of extrasolar planetary systems with more than one planet.

NAUENBERG M.

Abstract (from CDS):

Recent analysis of the Doppler-shift oscillations of the light from extrasolar planetary systems indicates that some of these systems have more than one large planet. In this case, it has been shown that the masses of these planets can be determined without the familiar ambiguity due to the unknown inclination angle of the plane of the orbit of the central star provided, however, that the star mass is known. A method is presented here that also determines a lower limit to the mass of this star from these observations. As an illustration, our method is applied to the Keck and Lick data for GJ 876.

Abstract Copyright: ∼

Journal keyword(s): Methods: Analytical - Stars: Planetary Systems

Simbad objects: 1

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Number of rows : 1
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 BD-15 6290 BY* 22 53 16.7325836486 -14 15 49.304052185 12.928 11.749 10.192 9.013 7.462 M3.5V 1106 1

Query : 2002ApJ...568..369N

Basic data :
BD-15 6290 -- BY Dra Variable
Other object types: otypes_help 		* (2015ApJS,BD,...), PM* (2013MNRAS,Ci,...), BY* (2017ARep), Ro* (2012A&A), V* (V*), NIR (2MASS), MIR (WISEA)
ICRS coord. (ep=J2000) : 		22 53 16.7325836486 -14 15 49.304052185 (Optical) [ 0.0338 0.0258 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) : 		22 50 34.6499284991 -14 31 14.052098435 [ 0.0338 0.0258 90 ]
Gal coord. (ep=J2000) : 		052.0040597500243 -59.6300891766021 [ 0.0338 0.0258 90 ]
Proper motions mas/yr : 		957.715 -673.601 [0.041 0.031 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz : 		V(km/s) -1.47 [0.0003] / z(spectroscopic) -0.000005 [0.000000] / cz -1.47 [0.00]
   (Opt) A 2018MNRAS.475.1960F
Parallaxes (mas): 		214.0380 [0.0356] A 2020yCat.1350....0G
Spectral type: 		M3.5V C 1983SAAOC...7..106W
Fluxes (12) :
U 12.928 [0.0034] B 2009AJ....137.4186L
B 11.749 [0.0017] B 2009AJ....137.4186L
V 10.192 [0.0017] B 2009AJ....137.4186L
R 9.013 [0.0017] B 2009AJ....137.4186L
G 8.875059 [0.002861] C 2020yCat.1350....0G
I 7.462 [0.0017] B 2009AJ....137.4186L
J 5.934 [0.019] C 2003yCat.2246....0C
H 5.349 [0.049] C 2003yCat.2246....0C
K 5.010 [0.021] C 2003yCat.2246....0C
g 10.919 [~] D 2012yCat.1322....0Z
r 9.872 [0.08] D 2012yCat.1322....0Z
i 8.296 [0.05] D 2012yCat.1322....0Z
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 4 		: 235 Display criteria :

Identifiers (43) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

BD-15 6290 GSC 05819-00957 NAME NC 59 UBV M 5470
Ci 20 1387 HIC 113020 NLTT 55130 UCAC2 26801725
CNS5 5644 HIP 113020 8pc 212.69A UCAC4 379-165686
EPIC 206019387 JP11 295 PLX 5546 V* IL Aqr
EPIC 206019392 Karmn J22532-142 PLX 5546.00 WEB 20121
GCRV 14365 LFT 1745 PM J22532-1415 WISEA J225317.42-141556.1
GEN# -0.01506290 LHS 530 Ross 780 Zkh 338
G 156-57A LPM 841 TIC 188580272 [RHG95] 3604
G 156-57 LTT 9244 TYC 5819-1255-1 Gaia DR3 2603090003484152064
GJ 876 2MASS J22531672-1415489 UBV 19209 Gaia DR2 2603090003484152064
GJ 876 A MCC 337 UBV 19610

References (1106 between 1850 and 2026) (Total 1106)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 11    Distance : 3    Var : 4    Rot : 5    Fe/H : 44    Plx : 6    PM : 10    SpT : 20   

   

Observing logs
Herschel : 3    ISO : 4   

   

External archives :

Link by name to the catalogue in VizieR :

BD-15 6290 G 156-57A G 156-57 GJ 876 GJ 876 A
GSC 05819-00957 HIC 113020 HIP 113020 LHS 530 2MASS J22531672-1415489
NLTT 55130 PLX 5546 TYC 5819-1255-1 UCAC2 26801725 UCAC4 379-165686
V* IL Aqr WISEA J225317.42-141556.1 Gaia DR3 2603090003484152064 Gaia DR2 2603090003484152064

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