Table 2: Stellar parameters taken from Allende Prieto & Lambert (1999). The first column gives the name of the planet followed by the stellar HD and HIP numbers. The other columns list the apparent visual magnitude, the parallax, the absolute magnitude, the colour B-V and the stellar mass, radius, bolometric correction and effective temperature. The rms errors are given below the parameter values except for the radius. Note that Allende Prieto & Lambert (1999) originally gave the radius as $\log R$ . Hence, the error stated below the calculated radius is the maximum deviation of the calculated value obtained by applying the rms error to the $\log R$ value.
Planet $V{\rm mag}$ plx $V{\rm MAG}$ B-V Mass $R_\star$ BC $\log T_{\rm eff}$

[mag] [mas] [mag] [mag] [ $M_{\odot}$ ] [ $R_{\odot}$ ] [mag] [K]

OGLE-TR-56 b

HD 83443 b 8.23 22.97 5.04 0.811 0.98 1 0.13 3.74

83443 0.9 0.17 0.01 0.05 0.01 0

47202

HD 46375 b 7.91 29.93 5.29 0.86 0.9 1 0.16 3.73

46375 1.07 0.16 0.01 0.05 0.01 0

31246

HD 187123 b 7.83 20.87 4.43 0.661 1.12 1.15 0.04 3.77

187123 0.71 0.15 0.1 0.05 0.03 0.01

97336

HD 179949 b 6.25 36.97 4.09 0.548 1.14 1.17 0.03 3.79

179949 0.8 0.1 0.07 0.03 0.02 0

94645

HD 209458 b 7.65 21.24 4.29 0.594 1.03 1.15 0.06 3.78

209458 1 0.21 0.11 0.08 0.02 0.01

108859

HD 75289 b 6.35 34.55 4.04 0.578 1 1.32 0.07 3.78

75289 0.56 0.07 0.1 0.06 0.02 0.01

43177

BD-10_3166 b

$\tau$ Boo b 4.5 64.12 3.53 0.508 1.3 1.41 -0.01 3.81

120136 0.7 0.05 0.12 0.07 0.03 0.01

67275

HD 76700 b 8.16 16.75 4.28 0.745 1 1.38 0.1 3.75

76700 0.66 0.17 0.09 0.1 0.03 0.01

43686

51 Peg b 5.45 65.1 4.52 0.666 1.01 1.15 0.08 3.76

217014 0.76 0.05 0.01 0.03 0 0

113357

HD 49674 b 8.1 24.55 5.05 0.729 0.95 0.95 0.11 3.75

49674 1.14 0.2 0.04 0.07 0 0

32916

$\upsilon$ And b 4.1 74.25 3.45 0.536 1.37 1.45 -0.03 3.81

9826 0.72 0.05 0.01 0.03 0 0

7513

**Table 2:** Stellar parameters taken from Allende Prieto & Lambert (1999). The first column gives the name of the planet followed by the stellar HD and HIP numbers. The other columns list the apparent visual magnitude, the parallax, the absolute magnitude, the colour B-V and the stellar mass, radius, bolometric correction and effective temperature. The rms errors are given below the parameter values except for the radius. Note that Allende Prieto & Lambert (1999) originally gave the radius as $\log R$ . Hence, the error stated below the calculated radius is the maximum deviation of the calculated value obtained by applying the rms error to the $\log R$ value.
Planet	$V{\rm mag}$	plx	$V{\rm MAG}$	B-V	Mass	$R_\star$	BC	$\log T_{\rm eff}$
	[mag]	[mas]	[mag]	[mag]	[ $M_{\odot}$ ]	[ $R_{\odot}$ ]	[mag]	[K]
OGLE-TR-56 b
HD 83443 b	8.23	22.97	5.04	0.811	0.98	1	0.13	3.74
83443		0.9	0.17		0.01	0.05	0.01	0
47202
HD 46375 b	7.91	29.93	5.29	0.86	0.9	1	0.16	3.73
46375		1.07	0.16		0.01	0.05	0.01	0
31246
HD 187123 b	7.83	20.87	4.43	0.661	1.12	1.15	0.04	3.77
187123		0.71	0.15		0.1	0.05	0.03	0.01
97336
HD 179949 b	6.25	36.97	4.09	0.548	1.14	1.17	0.03	3.79
179949		0.8	0.1		0.07	0.03	0.02	0
94645
HD 209458 b	7.65	21.24	4.29	0.594	1.03	1.15	0.06	3.78
209458		1	0.21		0.11	0.08	0.02	0.01
108859
HD 75289 b	6.35	34.55	4.04	0.578	1	1.32	0.07	3.78
75289		0.56	0.07		0.1	0.06	0.02	0.01
43177
BD-10_3166 b
$\tau$ Boo b	4.5	64.12	3.53	0.508	1.3	1.41	-0.01	3.81
120136		0.7	0.05		0.12	0.07	0.03	0.01
67275
HD 76700 b	8.16	16.75	4.28	0.745	1	1.38	0.1	3.75
76700		0.66	0.17		0.09	0.1	0.03	0.01
43686
51 Peg b	5.45	65.1	4.52	0.666	1.01	1.15	0.08	3.76
217014		0.76	0.05		0.01	0.03	0	0
113357
HD 49674 b	8.1	24.55	5.05	0.729	0.95	0.95	0.11	3.75
49674		1.14	0.2		0.04	0.07	0	0
32916
$\upsilon$ And b	4.1	74.25	3.45	0.536	1.37	1.45	-0.03	3.81
9826		0.72	0.05		0.01	0.03	0	0
7513

Source LaTeX | All tables | In the text

	1 Introduction
	2 Planetary and stellar parameters
	3 Model stellar wind regimes
	4 Estimation of the Poynting flux in the planetary magnetospheres
	5 Conclusions
	References