Table 1
Objects studied in the program.
HD | Other | V | Ka | Spectral | Parallaxb | |
number | identifier | type | [mas] | |||
|
||||||
6532 | CD-27 355 | 8.40 | 8.19 | A3 Sr Cr | 6.14 ± 1.03 | |
9289 | BD-11 286 | 9.40 | 8.87 | A3 Sr Eu Cr | ||
12932 | BD-19 384 | 10.36 | 9.46 | A4 Sr Eu | ||
19918 | CD-82 53 | 9.37 | 8.78 | A5 Sr Eu Cr | 4.07 ± 0.82 | |
24712 | HR 1217 | 5.99 | 5.26 | A9 Sr Eu Cr | 20.32 ± 0.39 | |
42659 | BD-15 1299 | 6.77 | 6.36 | A3 Sr Cr Eu | 7.60 ± 0.51 | |
86181 | CPD-58 1700 | 9.39 | 8.68 | F0 Sr | 3.49 ± 1.05 | |
99563 | BD-08 3173 | 8.2 | 7.74 | F0 Sr | 3.92 ± 1.15 | |
101065 | CD-46 7232 | 8.02 | 6.92 | F3 Ho | 8.93 ± 0.87 | |
116114 | BD-17 3829 | 7.03 | 6.35 | F0 Sr Cr Eu | 7.71 ± 0.55 | |
119027 | CD-28 10204 | 9.91 | 9.09 | A3 Sr Eu | ||
122970 | BD+06 2827 | 8.30 | 7.31 | F0 Cr Eu Sr | 8.67 ± 0.70 | |
134214 | BD-13 4081 | 7.47 | 6.67 | F2 Sr Eu Cr | 9.74 ± 0.64 | |
137949 | BD-16 4093 | 6.68 | 6.25 | F0 Sr Eu Cr | 11.28 ± 0.67 | |
150562 | CD-48 11127 | 9.95 | 8.88 | A5: Eu Si? | ||
154708 | CD-57 6753 | 8.76 | 7.95 | A2 Sr Eu Cr | 6.75 ± 0.96 | |
161459 | CD-51 11145 | 10.4 | 9.54 | A2 Eu Sr Cr | ||
166473 | CD-37 12303 | 7.92 | 7.45 | A5 Sr Eu Cr | ||
176232 | HR 7167 | 5.91 | 5.30 | A6 Sr | 12.76 ± 0.29 | |
185256 | CD-30 17252 | 9.92 | 8.92 | F0 Sr Eu | ||
190290 | CD-79 800 | 9.89 | 9.18 | A0 Eu Sr | ||
193756 | CD-52 9483 | 9.19 | A9 Sr Cr Eu | |||
196470 | BD-18 5731 | 9.79 | 9.17 | A2 Sr Eu | ||
201601 | HR 8097 | 4.71 | 4.01 | A9 Sr Eu | 27.55 ± 0.62 | |
203932 | CD-30 18600 | 8.82 | 8.13 | A5 Sr Eu | ||
213637 | BD-20 6447 | 9.58 | 8.54 | F1 Eu Sr | ||
217522 | CD-45 14901 | 7.53 | 6.63 | A5 Sr Eu Cr | 11.36 ± 0.79 | |
218495 | CD-64 1414 | 9.34 | 9.03 | A2 Eu Sr | ||
|
||||||
Magnetic Ap stars | ||||||
|
||||||
40711 | BD+10 973 | 8.58 | 8.15 | A0 Sr Cr Eu | 2.66 ± 0.95 | |
55719 | HR 2727 | 5.31 | 5.14 | A3 Sr Cr Eu | 7.93 ± 0.38 | |
59435 | V827 Mon | 7.97 | 6.39 | A4 Sr Cr Eu | 2.70 ± 0.76 |
Notes. In Col. 1, we give the HD number of the objects, in Col. 2 another identifier, in Cols. 3 and 4 the magnitudes in V and K bands, in Col. 5 the spectral type, and finally in Col. 6 the parallax. Most information was collected from the SIMBAD database, except for the spectral types, which are from Renson & Manfroid (2009), and the parallaxes, obtained from van Leeuwen (2007).
For some targets, Leeuwen (2007) does not list a parallax.
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