Table A.1.
List of long-period Ap stars found by our technique in the TESS Sectors 14−26 data, obtained in the second year of mission operations and covering the northern ecliptic hemisphere.
Spectral | Lines(a) | TESS | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
TIC | HD/Other id | type | V | Teff | log g | roAp | ⟨Bz⟩rms/B0/Q0 | Refs | Prot | Refs | v sin i | Refs | Notes | sectors |
(mag) | (K) | (cm s−2) | (kG) | (d) | (km s−1) | |||||||||
2689133 | HD 242800 | A0p Si | 10.55 | 8500 | 4.0 | S19 | ||||||||
2849758 | HD 243007 | A1p Si | 10.2 | 9000 | 3.6 | δ Sct star | S19 | |||||||
21073591 | BD+29 3448 | A9p Sr | 9.54 | 7600 | 3.6 | δ Sct star | S14 | |||||||
26749633 | KIC 11031749 | 12.50 | 7000 | 3.9 | roAp | S14,15 | ||||||||
29715050 | TYC 2653-2787-1 | A0p HgSi | 9.08 | 10450 | 4.2 | S14 | ||||||||
40564267 | HD 184471 | A9p SrCrEu | 9.00 | 7750 | 3.6 | 0.5/–/– | 4 | 50.8 | 4 | s | 3 | δ Sct star | S14 | |
44488067 | HD 2453 | A1p SrEuCr | 6.91 | 8900 | 3.8 | 0.8/3.7/4.3 | 1 | 521 | 12 | r | 1 | S17 | ||
76379777 | HD 247591 | A1p SiCrSr | 10.47 | 9900 | 3.8 | S19 | ||||||||
77038207 | HD 96003 | A3p SrCr | 6.87 | 9500 | 3.9 | 0.2/–/– | 5, 6 | < 20 | 5 | S22 | ||||
77128654 | HD 97127 | 9.43 | 6700 | 4.0 | roAp | S22 | ||||||||
78784187 | HD 249401 | A2p Si | 10.83 | 8150 | 3.6 | δ Sct/γ Dor star? | S19 | |||||||
115054217 | HD 244545 | A1p Si | 10.37 | 8350 | roAp? | EB | S19 | |||||||
115201166 | HD 244640 | A0p SiSr | 9.94 | 9650 | 4.0 | roAp? | S19 | |||||||
115820611 | HD 245416 | A2p CrSi | 9.71 | 8150 | 3.7 | S19 | ||||||||
116144208 | HD 245726 | A1p SiSr | 10.8 | 8750 | 3.6 | S19 | ||||||||
116995376 | TYC 2413-476-1 | A0p Sr | 10.82 | 9050 | 3.8 | δ Sct star? | S19 | |||||||
127755719 | HD 243321 | A0p Si | 9.61 | 10000 | 3.9 | S19 | ||||||||
127755856 | BD+32 976 | A2p Sr | 10.28 | 7600 | 4.2 | roAp? | S19 | |||||||
127959761 | HD 35436 | A1p SiSr | 9.55 | 8000 | 3.5 | δ Sct star | S19 | |||||||
154786038 | HD 96571 | A2p SrEu | 7.31 | 8100 | 3.6 | δ Sct star? | S14,19,20,26 | |||||||
155667362 | HD 276625 | A7p CrEu | 9.94 | 7100 | 3.9 | S19 | ||||||||
158216369 | KIC 7018170 | 13.28(b) | 6950 | 4.0 | roAp | 72.7 | 13 | S14 | ||||||
158275114 | BD+44 3063 | A5p EuCr | 10.19 | 7450 | 4.0 | roAp | –/3.2/– | 7 | r; 4.2 | 2 | S14,26 | |||
163801263 | HD 203922 | A2p SrCrEu | 8.50 | 7600 | 3.6 | S15 | ||||||||
165327084 | HD 110066 | A1p SrCrEu | 6.385 | 9000 | 3.9 | 0.1/4.1/– | 1 | 4900? | 14 | r | 1 | S22 | ||
165446000 | BD+39 4435 | F0p SiSrCr | 9.3 | 7700 | S15 | |||||||||
176902576 | HD 222416 | A0p SiSr | 7.73 | 9850 | 3.9 | S17 | ||||||||
185716313 | HD 191742 | A5p SrCr | 8.16 | 8400 | 3.6 | 0.6/–/1.8 | 8, 9 | s; 6 | 3, 9 | δ Sct star? | S14,15 | |||
198781718 | BD+29 3427 | A6p CrSr | 9.66 | 8000 | 4.2 | S14 | ||||||||
202899762 | BD+46 570 | Ap SrEuCr | 9.63 | 7350 | 3.6 | S18 | ||||||||
207468665 | HD 148330 | A2p SiSr | 5.734 | 9700 | 3.8 | 0.3/–/– | 10 | 4.288(c) | 10 | (s); 11.6 | 3, 10 | S16,19,23,25 | ||
233539061 | HD 174016 | (d) | 7.45 | 6225 | All but S18 | |||||||||
238659021 | HD 8441 | A2p Sr | 6.676 | 9200 | 0.1/–/– | 11 | 69.51 | 15 | s | 3 | δ Sct star | S17 | ||
239801694 | HD 247628 | A5p SiSr | 10.59 | 9050 | 4.1 | S19 | ||||||||
251282995 | HD 18078 | A0p SrCr | 8.27 | 8500 | 3.4 | roAp? | 0.7/3.5/– | 1358 | 16 | r | 1 | S18 | ||
251976407 | HD 221568 | A1p SrCrEu | 7.55 | 9500 | 3.9 | 0.7/–/– | 6 | 159.1 | 15 | s | 3 | S17,24 | ||
274242788 | HD 92728 | A0p Si | 5.782 | 10050 | 3.9 | 22 | 21 | S21 | ||||||
286462756 | HD 335238 | A1p CrEu | 9.26 | 9350 | 4.2 | 1.4/9.3/11.9 | 1 | 48.7 | 1 | r | 1 | S15 | ||
286965228 | HD 127304 | B9p Si? | 6.05 | 9950 | 4.1 | S23 | ||||||||
286992225 | TYC 2553-480-1 | A2p SrEu | 11.56 | 7500 | 4.3 | roAp | S23 | |||||||
289548946 | BD+47 3253 | A0p Si | 9.55 | 8800 | 4.0 | S15,16 | ||||||||
298197561 | HD 340577 | A3p SrCrEu | 9.09 | 8450 | 3.5 | 116.7 | 17 | δ Sct star | S14,15 | |||||
301918605 | HD 17330 | B7p Si | 7.11 | 10250 | 0.6/–/– | 5, 6 | 23 | 6 | S18 | |||||
301946105 | HD 7410 | A7p CrEu | 9.07 | 7800 | 3.5 | S17 | ||||||||
312221714 | HD 248727 | A0p MnSiCr | 10.34 | 9800 | 3.9 | δ Sct star? | S19 | |||||||
327293700 | HD 9996 | B9p CrEuSi | 6.38 | 10500 | 4.0 | 0.7/4.7/– | 1 | 7850 | 15 | r | 1 | S18 | ||
331644554 | BD+46 3543 | A2p Si | 9.75 | 8450 | 4.3 | δ Sct star; EB | S16 | |||||||
341616734 | HD 89069 | A0p SrCrEu | 8.42 | 9550 | 4.0 | 0.5/–/– | 5 | 19 | 18 | s; < 20 | 3, 5 | S14,20,21,26 | ||
343126267 | BD+54 2730 | F0p SiSr | 10.46 | 8000 | 4.2 | δ Sct star | S16,17 | |||||||
346595127 | HD 22860 | B9p Si | 6.86 | 10700 | 4.1 | 6.27(e) | 19 | S18 | ||||||
347202840 | HD 236298 | A0p Si | 9.45 | 10700 | 4.2 | S17,24 | ||||||||
352787151 | BD+35 5094 | F0p SrEu | 9.08 | 6900 | 3.5 | roAp? | S17 | |||||||
353371885 | HD 249931 | A0p SiSr | 10.62 | 9100 | 4.3 | S19 | ||||||||
368073692 | HD 278204 | B5p Si | 10.45 | 10850 | 4.1 | S19 | ||||||||
371976932 | HD 240242 | A4p Si | 10.15 | δ Sct star | S17,24 | |||||||||
373378410 | BD+35 4488 | A2p SiSr | 9.83 | 8750 | 4.0 | S15 | ||||||||
379529618 | HD 12288 | A2p CrSi | 7.74 | 8800 | 3.8 | 1.6/8.0/– | 1 | 34.9 | 20 | r | 1 | S18,19,25 | ||
389105232 | BD+57 2636 | Ap SrCrEu | 9.55 | 7900 | 3.8 | S16,17 | ||||||||
391462523 | HD 187400 | A0p Si | 8.63 | 9100 | 4.1 | S14 | ||||||||
403625657 | HD 11187 | A0p SiCrSr | 7.94 | 10750 | 3.5 | 0.6/–/– | (s) | 3 | S18 | |||||
408211646 | HD 332312 | A4p Sr | 9.72 | 8650 | 3.5 | S14,15 | ||||||||
409522234 | HD 14437 | B9p CrEuSr | 7.27 | 10450 | 3.9 | 1.9/7.6/– | 1 | 26.87 | 20 | r | 1 | S18 | ||
430355895 | BD+52 3124 | A0p Si | 10.12 | 9050 | 4.0 | roAp? | S16,17 | |||||||
450217536 | TYC 3729-816-1 | F0p SrSi | 11.35 | 6650 | 3.6 | S19 | ||||||||
468507699 | HD 206977 | A5p SrEu | 8.98 | 8650 | 3.8 | S15,16 | ||||||||
470837956 | BD+61 2565 | A8p SrEuCr | 9.9 | 8200 | 3.4 | roAp? | S17,18 | |||||||
470878580 | BD+65 1981 | Ap Si | 10.09 | 10550 | 4.3 | roAp? | S17,18,24 |
Notes.
V magnitude from Zacharias et al. (2004).
TESS photometry definitely does not show any low-frequency variability; the published period may be spurious.
SB2 system; HD 174017 (secondary) is the Ap component (A0p SrCrEu); HD 174016 is a G6III star (Renson & Manfroid 2009), unresolved by speckle interferometry (Hartkopf & McAlister 1984; Horch et al. 2015).
TESS photometry shows variations with a period of , which is typical of rotation, but the amplitude is very low and the period is not an alias of the published value.
References. (1) Mathys (2017); (2) Balona et al. (2011); (3) this paper; (4) Kudryavtsev & Romanyuk (2012); (5) Romanyuk et al. (2017); (6) Romanyuk et al. (2018); (7) Balona et al. (2011); (8) Babcock (1958); (9) Preston (1971); (10) Ziznovsky & Romanyuk (1990); (11) Aurière et al. (2007); (12) Mathys et al. (1997); (13) Hey et al. (2019); (14) Adelman (1981); (15) Pyper & Adelman (2017); (16) Mathys et al. (2016); (17) Hümmerich et al. (2016); (18) Netopil et al. (2017); (19) Wraight et al. (2012); (20) Wade et al. (2000); (21) Zorec & Royer (2012).
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