Table 3.
Stars with moderately long rotation periods (20 d ≲ Prot ≲ 50 d) found in the TESS Cycles 3 and 4 data.
| Spectral | Lines (b) | TESS | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| TIC | HD | type | V | Teff(a) | log g(a) | roAp | ⟨Bz⟩rms/B0/Q0 | Refs. | Prot | Plitt | Refs. | v sin i | Refs. (c) | Notes | sectors |
| (mag) | (K) | (cm s−2) | (kG) | (d) | (d) | (km s−1) | |||||||||
| 2934856 | 281056 | A5- | 10.68 | 8910 | 3.45 | 34.0 | 34.3 | 1 | 43–45 | ||||||
| 96855460 | 185256 | F0p SrEu | 9.96 | 7100 | 4.00 | roAp | 0.7/–/1.4 | 2, 3 | 25.64 | 5.5 | 3 | 27 | |||
| 162027140 | 97394 | A5p EuCrSr | 8.76 | 8360 | 3.75 | –/3.1/– | 4 | 47.38 | r | 4 | 36–37 | ||||
| 276300910 | 134799A | A7p SrCrMg | 7.94 | 7840 | 4.25 | 22.6 | 25.373 | 1 | δ Sct (d) | 38 | |||||
| 286255541 | 69913 | B9p Si | 8.20 | 9880 | 3.50 | 19.98 | 19.975 | 5 | 34–36 | ||||||
| 312839768 | 122525 | A0p EuSrCr | 8.71 | 8330 | 3.55 | –/–/1.7 | 6 | 26.70 | 26.072 | 7 | 7 | 6 | 38 | ||
| 427032468 | 140748 | A2p EuCr | 9.22 | 8490 | 3.80 | 50.8 | 36.52 | 1 | vs | F | 39 | ||||
| 429553678 | 40678 | A0p SiSr | 7.38 | 9520 | 3.70 | 26.9 | 22.029 | 7 | 44 |
Notes. Columns 1–9 are the same in Table 2, in which Col. 10 has no counterpart. It contains the values of the moderately long periods that were determined in the course of this study (see Sect. 2.4.2). The data presented in Cols. 11–16 of are of the same nature as those given in Cols. 10–15 of Table 2.
F: the line width information is based on visual inspection of a FEROS spectrum of our collection.
The δ Sct pulsation signal probably originates from the companion, HD 134799B. See text for details.
References. (1) Netopil et al. (2017); (2) Hubrig et al. (2004); (3) Kochukhov et al. (2013); (4) Elkin et al. (2011); (5) Bernhard et al. (2015a); (6) Ryabchikova & Romanovskaya (2017); (7) Hümmerich et al. (2016).
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