Table 3:

The sample of UMa group members.

Object

Spectral type

V

Montes01b

King03

Fuhrmann04

Sub-sample

[mas]

pec. vel.

rad. vel.

kin.

phot.

final

HD 11131

G1V

1

42.35 0.873

Y

Y

?

Y?

Y?

Y

M01k

HD 24916 A

K4V

63.41 2.00

Y

Y

N?

?

N?

M01k

HD 26923

G0IV

1

47.20 1.08

Y

Y

Y?

Y

Y?

Y

M01k

HD 28495

G0V

36.32 1.07

N

Y

Y

Y

Y

K03k

K03f

HD 38393

F7V

111.49 0.60

Y

Y

?/Y?

Y?

Y?

M01k

HD 39587

G0V

1

115.43 1.08

Y

Y

Y

Y

K03k

K03f

HD 41593

K0V

1

64.71 0.91

Y

Y

N?/?

Y

N?/?

Y

M01k

HD 59747

G5V

1

50.80 1.29

Y

Y

Y

Y?

Y

Y

M01k

K03k

K03f

HD 71974 A

G5V

34.83 1.37

Y

N

Y

Y?

Y

K03k

K03f

HD 95650

M0

85.76 1.36

N

Y

Y

Y?

Y

K03k

K03f

HD 238087

K5

35.24 1.24

Y

Y

Y?

?

?

M01k

HD 109011

K2V

42.13 3.11

Y

Y

Y

K03k

K03f

HD 109647

K0V

38.08 1.11

Y

Y

Y

Y

Y

M01k

K03k

K03f

HD 110463

K3V

43.06 0.82

Y

Y

Y

Y

Y

M01k

K03k

K03f

HD 112196

F8V

29.19 1.60

Y

Y

N?/?

?

N?/?

M01k

HD 115043

G1Va

38.92 0.67

Y

Y

Y

Y

Y

M01k

K03k

K03f

HD 238224

K5

39.84 1.44

Y

Y

Y

?

Y?

M01k

K03k

HD 152863 A

G5III

7.14 0.67

Y

Y

?

Y?

?

M01k

HD 155674 A

K0

47.14 1.88

Y

Y

?

?

?

M01k

HD 155674 B

K8

47.86 3.11

Y

Y

?

?

?

M01k

HD 167389

F8

29.91 0.59

Y

Y

N?

?

N?/?

M01k

HD 171746 A

G2V

2

29.23 1.54

N

Y

Y

Y?

Y

K03k

K03f

HD 171746 B

G2V

2

29.23 1.54

Y

Y?

Y

K03k

K03f

HD 184960

F7V

39.08 0.47

Y

Y

?/Y?

?

?/Y?

M01k

HD 205435

G8III

26.20 0.51

Y

Y

?/Y?

?

?

M01k

The table gives the spectral type (2), the V band magnitude (3) derived from the Hipparcos system using the conversion of Bessell (2000) in most cases, the parallax (4), Eggen's peculiar velocity criterion (5) and Eggen's cluster radial velocity criterion (6) as applied by Montes01b, the kinematic UVW criterion (7), photometric criterion (8), and final membership according to King03 (9), and the spectroscopic membership following Fuhrmann04 (10). The last column indicates the membership of the sub-samples M01k, K03k, and K03f as described in the text in detail. Most astrometric and photometric measurements are taken from the Hipparcos catalogue (Perryman et al. 1997). Exceptions are indicated in the footnote below.
¹ Fuhrmann04. ² Based on values in the Hipparcos system given by Fabricius & Makarov (2000). See Sect. 3.3 for more details. ³ According to Fuhrmann04, the parallax of the primary HD 11171 is adopted.