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Table 1

The sample of 12 stars.

Star HR HD V (B − V ) Spectral type* Prime reason(s) for
(mag) (mag) inclusion in G+2003

21 LMi 3974 87696 4.7 0.18 A7 V(n) AM; inconsistent UV flux
4875 111604 6.0 0.15 A8 Vn kA1.5 mA1.5 λ Boo AM; variable RV
λ Boo 5351 125162 3.2 0.08 A3 Va kB9mB9 λ Boo Gray classification
5368 125489 6.4 0.20 A7 Vn AM; inconsistent UV flux
12 Ser 5770 138527 6.2 −0.04 B9 IV (λ Boo) AM; Hipparcos double
6878 169009 6.5 0.12 B9 V He wk (CP) AM; variable RV
λ Aql 7236 177756 3.4 −0.09 B9 IV (He wk) (CP) AM; variable RV
7288 179791 6.6 0.09 A1.5 IVn Inconsistent UV flux
35 Aql 7400 183324 5.8 0.08 A0 Vb λ Boo Gray classification
7903 196821 6.1 −0.05 A0 III+p kB8 mA1 (CP) AM; UV flux
τ Peg 8880 220061 4.8 0.17 A8 V(n) kA5mA5 (λ Boo) AM; variable RV
15 And 8947 221756 5.6 0.10 A1 Va λ Boo Gray classification

Notes. (λ Boo) indicates marginal classification.

(†)

Included in the list of Abt & Morrell (1995).

(*)

This paper, except for λ Boo (Gray et al. 2003).

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