Table 1.
Ba star systems to which our methodology was applied.
BD/HD | HIP | Type | MBa [M⊙] | [Fe/H] | RV ref. ( * ) | HD | HIP | Type | MBa [M⊙] | [Fe/H] | RV ref. ( * ) |
---|---|---|---|---|---|---|---|---|---|---|---|
−10°4311 | 80356 | preRGB | 0.8 ± 0.1 | −0.65 | E19 | 95241 | 53791 | preRGB | 1.3 ± 1.1 | −0.37 | E19,M04 |
−11°3853 | 73444 | preRGB | 0.85 ± 0.04 (1) | −0.94 (1) | E19 | 98991 | 55598 | preRGB | 1.45 ± 0.08 | −0.44 | E19 |
−14°2678 | 43527 | mBag | 3.0 ± 0.2 | 0.01 | U98a | 104979 | 58948 | mBag | 2.7 ± 0.2 | −0.26 | J19,M90 |
2454 | 2235 | preRGB | 1.23 ± 0.07 (1) | −0.29 (1) | E19,M04 | 107541 | 60292 | sBag | 1.1 ± 0.2 | −0.63 | U98b |
5424 | 4347 | sBag | 1.3 ± 0.4 | −0.43 | U98a | 107574 | 60299 | preRGB | 1.11 ± 0.05 | −0.80 | E19 |
16458 | 13055 | sBag | 1.9 ± 0.1 | −0.64 | M90 | 119185 | 66844 | mBag | 1.7 ± 0.2 | −0.42 | J19,U98a |
18182 | 13596 | mBag | 1.8 ± 0.2 | −0.17 | J19 | 121447 | 68023 | sBag | 1.6 ± 0.1 | −0.90 | J95 |
20394 | 15264 | sBag | 2.0 ± 0.2 | −0.27 | G96 | 123585 | 69176 | preRGB | 1.0 ± 0.1 (0) | −0.50 | E19 |
24035 | 17402 | sBag | 1.3 ± 0.3 | −0.23 | U98a | 123949 | 69290 | sBag | 1.3 ± 0.3 | −0.23 | J19,U98a |
27271 | 20102 | mBag | 2.9 ± 0.2 | −0.07 | U98b,M04 | 127392 | 71058 | preRGB | 0.8 ± 0.3 | −0.52 | E19 |
31487 | 23168 | sBag | 2.5 ± 0.2 (2) | −0.04 (2) | M90 | 139195 | 76425 | mBag | 2.6 ± 0.1 | −0.07 | M90,G91 |
34654 | 25222 | preRGB | 1.19 ± 0.05 (0) | −0.09 | E19 | 143899 | 78681 | mBag | 2.4 ± 0.1 | −0.29 | U98a |
40430 | 28265 | mBag | 2.3 ± 0.2 | −0.34 | J19 | 178717 | 94103 | sBag | 1.6 ± 0.9 | −0.52 | M90 |
43389 | 29740 | sBag | 1.8 ± 0.4 | −0.35 | U98b | 180622 | 94785 | mBag | 1.8 ± 0.3 | 0.03 | U98b |
44896 | 30338 | sBag | 3.0 ± 1.2 (0) | −0.25 | U98b | 182274 | 95293 | preRGB | 1.09 ± 0.05 | −0.32 | E19,M04 |
49641 | 32713 | sBag | 2.7 ± 1.2 | −0.3 | M90 | 183915 | 96024 | sBag | 1.8 ± 1.0 | −0.59 | J19,J98 |
49841 | 32831 | mBag | 2.85 ± 0.10 (0) | 0.2 | U98b | 199939 | 103546 | sBag | 2.7 ± 0.4 (0) | −0.22 | M90,M04 |
50082 | 32960 | sBag | 1.6 ± 0.3 | −0.32 | U98b | 200063 | 103722 | mBag | 2.0 ± 1.3 | −0.34 | U98b |
50264 | 32894 | preRGB | 0.9 ± 0.1 (0) | −0.34 | E19 | 201657 | 104542 | sBag | 1.8 ± 0.5 | −0.34 | U98b |
51959 | 33628 | mBag | 1.2 ± 0.1 | −0.21 | J19 | 201824 | 104684 | sBag | 1.7 ± 0.4 | −0.40 | G96 |
53199 | 34143 | mBag | 2.5 ± 0.1 | −0.20 | J19,M04 | 202400 | 105294 | preRGB | 0.98 ± 0.08 (3) | −0.7 (3) | N20 |
58121 | 35935 | mBag | 2.6 ± 0.5 | −0.01 | U98b | 204075 | 105881 | mBag | 4.5 ± 0.3 | −0.09 | M90 |
58368 | 36042 | mBag | 2.6 ± 0.2 | 0.04 | M90 | 205011 | 106306 | mBag | 1.8 ± 0.3 | −0.26 | J98,M90 |
59852 | 36613 | mBag | 2.5 ± 0.3 | −0.22 | U98a | 207585 | 107818 | preRGB | 0.90 ± 0.10 (0) | −0.57 | E19 |
77247 | 44464 | mBag | 3.9 ± 0.2 | −0.13 | M90 | 210946 | 109747 | mBag | 1.8 ± 0.5 | −0.29 | U98b,M04 |
87080 | 49166 | preRGB | 1.38 ± 0.15 (0) | −0.60 | E19 | 211594 | 110108 | sBag | 2.0 ± 0.3 | −0.29 | U98b |
88562 | 50006 | sBag | 1.0 ± 0.1 | −0.53 | U98a | 216219 | 112821 | preRGB | 1.45 ± 0.1 | −0.17 | E19 |
91208 | 51533 | mBag | 2.3 ± 0.2 | −0.16 | U98a | 218356 | 114155 | mBag | 4.3 ± 1.1 | −0.06 | G06,U98b |
92626 | 52271 | sBag | 3.1 ± 0.6 | −0.15 | U98b | 221531 | 116233 | preRGB | 1.2 ± 0.1 (0) | −0.30 | E19 |
95193 | 53717 | mBag | 2.7 ± 0.1 | −0.04 | U98a | 224621 | 118266 | preRGB | 0.85 ± 0.06 (0) | −0.4 | N20 |
Notes. Column 1 lists the most commonly used identifiers, while Col. 2 lists the HIPPARCOS identifiers. Column 3 lists the Ba star type, which can be preRGB for stars classified as dwarfs or subgiants, or mBag or sBag for stars classified as mild or strong Ba giants, respectively. Column 4 lists the primary star masses and Col. 5, the metallicity of the system. These values were derived or collected by Escorza et al. (2019a) or Jorissen et al. (2019) for preRGB and giant systems, respectively, unless otherwise indicated. Finally, the last column gives the sources of the archival RV data we used. ( * )RV reference abbreviations: E19: Escorza et al. (2019a), U98a: Udry et al. (1998a), M04: Moultaka et al. (2004), M90: McClure & Woodsworth (1990), J19: Jorissen et al. (2019), G96: Griffin et al. (1996), U98b: Udry et al. (1998b), J98: Jorissen et al. (1998), J95: Jorissen et al. (1995), G91: Griffin (1991), N20: North et al. (2020), G06: Griffin (2006). Mass and metallicity references: (0)This work; (1)Bensby & Lind (2018); (2)Karinkuzhi et al. (2018); (3)North et al. (2020).
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