Table 5
Overview of spot latitudes in comparable targets sorted according to the spectral type of the stars.
| Star | Sp. type | P rot | Spots | Note | Ref. |
|
|
|||||
| τ Booa | F7 V |
|
L-H | 1–3 | |
| AE Phe B | F8 V |
|
L-M, (P) | B | 4–6 |
| σ2 CrB A | F9 V |
|
H,P | B | 7 |
| HD 307938 | G2 V |
|
(L)-P | 8, 9 | |
| LQ Lup | G2V-IV |
|
(L)-P | 10 | |
| HII 3163 | K0 V |
|
L, P | 11 | |
| AB Dor | K0 V |
|
L-P | 12–22 | |
| HII 686 | K4 V |
|
L,M,P | 11 | |
| LO Peg | K5-7 V |
|
(L)-P | 23–25 | |
Notes. In the “Spots” column P = polar, H = high-latitude, M = mid-latitude, and L = low-latitude. Parenthesis around the letter are used when spots are not always present in that latitude range or are weak. The binarity is stated in the “Note” column with “B”.
Reference. (1) Catala et al. (2007); (2) Donati et al. (2008); (3) Fares et al. (2009); (4) Maceroni et al. (1991); (5) Maceroni et al. (1994); (6) Barnes et al. (2004); (7) Strassmeier & Rice (2003); (8) Marsden et al. (2004); (9) Marsden et al. (2005); (10) Donati et al. (2000); (11) Stout-Batalha & Vogt (1999); (12) Kürster et al. (1994); (13) Collier-Cameron & Unruh (1994); (14) Collier Cameron (1995); (15) Unruh et al. (1995); (16) Hussain et al. (1997); (17) Unruh & Collier Cameron (1997); (18) Donati & Collier Cameron (1997); (19) Donati et al. (1999); (20) Collier Cameron et al. (1999); (21) Donati et al. (2003); (22) Jeffers et al. (2007); (23) Lister et al. (1999); (24) Barnes et al. (2005b); (25) Piluso et al. (2008).
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