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Table 1

Wide binary systems consisting of two main-sequence cool stars with at least one exoplanet for which X-ray data has been collected.

Star Spec. type BV Ang. sep. Dist. MP Porb asem log LX Apparent age J Jorb htide/hscale
(arcsec) (pc) (d) (MJup) (d) (AU) (erg s-1) (kg m2 d-1) (kg m2 d-1)

HD 189733 A K0V 0.93 11.2′′ 19.3 12 1.14 2.22 0.031 –4.501 28.2 1–2 Gyr 9.3e46 1.3e47 0.008
HD 189733 B M4V 11.2′′ 19.3 26.7 5 Gyr
CoRoT-2 A G7V 0.854 4′′ 270 4.5 3.31 1.74 0.028 –4.331 29.2 0.1–0.3 Gyr 4.3e47 4.0e47 0.072
CoRoT-2 B K9V 4′′ 270 27.0 5 Gyr
τ Boo A F7V 0.52 2.5′′ 15.0 3.3 8.14 3.31 0.048 –4.70 28.8 1–2 Gyr 2.0e48 1.5e48 0.047
τ Boo B M 2.5′′ 15.0 27.65 1–3 Gyr
υ And A F8IV-V 0.53 52′′ 13.5 9.5 0.62 4.62 0.059 –5.04 27.7 5 Gyr 6.4e47 1.4e47 0.002
υ And B M4V 52′′ 13.5 26.45 5 Gyr
55 Cnc A G8V 0.87 81′′ 13 43 0.026 0.74 0.015 –5.04 27.07 5 Gyr 4.6e46 2.3e45 0.005
55 Cnc B M3-4V 81′′ 13 26.22 5 Gyr

Notes. The closest exoplanet is given in case of multiple exoplanets per system.

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