2011A&A...525A.152M


C.D.S. - SIMBAD4 rel 1.7 - 2019.07.19CEST02:29:57

2011A&A...525A.152M - Astronomy and Astrophysics, volume 525A, 152-152 (2011/1-1)

Stellar wobble caused by a nearby binary system: eccentric and inclined orbits.

MORAIS M.H.M. and CORREIA A.C.M.

Abstract (from CDS):

Most extrasolar planets currently known were discovered by means of an indirect method that measures the stellar wobble caused by the planet. We previously studied a triple system composed of a star and a nearby binary on circular coplanar orbits. We showed that although the effect of the binary on the star can be differentiated from the stellar wobble caused by a planet, because of observational limitations the two effects may often remain indistinguishable. Here, we develop a model that applies to eccentric and inclined orbits. We show that the binary's effect is more likely to be mistaken by planet(s) in the case of coplanar motion observed equator-on. Moreover, when the orbits are eccentric, the magnitude of the binary's effect may be larger than in the circular case. Additionally, an eccentric binary can mimic two planets with orbital periods in the ratio 2/1. However, when the star's orbit around the binary's center of mass has a high eccentricity and a reasonably well-constrained period, it should be easier to distinguish the binary's effect from a planet.

Abstract Copyright:

Journal keyword(s): technique: radial velocities - celestial mechanics - planetary systems - binaries: general

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 HD 188753 ** 19 54 58.3717655 +41 52 17.529759   8.22   6.9   G9V 121 1
2 HD 196885 PM* 20 39 51.8753142885 +11 14 58.702911143   6.92 6.385 6.32   F8V 150 1
3 HD 196885B * 20 39 51.90 +11 14 59.0     13.0     M1V 12 1
4 * gam Cep SB* 23 39 20.9015326708 +77 37 56.505477975 5.190 4.250   2.6   K1III-IVCN1 541 1

    Equat.    Gal    SGal    Ecl

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2019.07.19-02:29:57

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