2018PASP..130h4201P


Query : 2018PASP..130h4201P

2018PASP..130h4201P - Publ. Astron. Soc. Pac., 130, part no 8, 4201-84201 (2018/August-0)

Variability analysis of δ Scuti candidate stars.

PAKSTIENE E., JANULIS R., TAUTVAISIENE G., DRAZDAUSKAS A., KLEBONAS L., MIKOLAITIS S., MINKEVICIUTE R. and BAGDONAS V.

Abstract (from CDS):

The Hipparcos catalog contains stars suspected to be δ Scuti variables for which extensive ground-based observations and characterization of variability are necessary. Our aim was to characterize variability of 13 candidates to δ Scuti type stars. We obtained 24 215 CCD images and analyzed stellar light curves using the Period04 program. Twelve δ Scuti candidate stars have been characterized as pulsating with frequencies intrinsic to δ Scuti stars: HIP 2923, HIP 5526, HIP 5659, HIP 11090, HIP 17585, HIP 74155, HIP 101473, HIP 106219, HIP 107786, HIP 113487, HIP 115093, and HIP 115856. Five of them (HIP 2923, HIP 5526, HIP 11090, HIP 115856, and HIP 106219) may be hybrid δ Scuti-γ Doradus pulsators. One more candidate, HIP 106223, is a variable star with longer periods of pulsations which are intrinsic to γ Doradus.

Abstract Copyright: © 2018. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s):

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 3397 * 00 37 03.5560574016 +31 29 11.300155764   7.95 7.65     F0III 24 0
2 TYC 2275-1038-1 * 00 37 13.0881617112 +31 25 09.408978768   11.49 10.86     ~ 1 0
3 TYC 1753-1926-1 * 01 10 00.0218012928 +27 59 22.547510916   11.46 11.07     ~ 1 0
4 HD 6988 * 01 10 43.3077344304 +27 52 04.593983016   8.49 8.10     F0 21 0
5 HD 7102 ** 01 12 41.26289 +65 00 32.8261           F0 22 0
6 TYC 4038-716-1 * 01 14 25.4664071400 +65 15 59.771266164   10.93 9.70     ~ 2 0
7 HD 14573 * 02 22 21.1305483528 +41 10 30.820971720   8.98 8.51     F5 8 0
8 HD 14622 PM* 02 22 50.3034199104 +41 23 46.657521456   6.063 5.795     F0III-IV 60 0
9 HD 23005 PM* 03 46 00.9400234704 +67 12 05.768204220   6.122 5.782     F1IVnn 42 0
10 TYC 4075-932-1 PM* 03 47 15.1386402552 +66 57 14.764064040   11.41 10.54     ~ 3 0
11 BD+70 825 * 15 08 30.8482581288 +69 42 02.031846732   11.23 10.54     ~ 2 0
12 HD 135119 * 15 09 06.2352460752 +69 39 11.114092980   7.42 7.12     F2 19 0
13 HD 195922 * 20 33 53.7099736560 +10 03 35.106338628   6.625 6.536     A2Vnn 31 0
14 BD+09 4580 * 20 34 02.3329203864 +10 15 11.416737672   9.92 8.79     K2 3 0
15 HD 204879 * 21 30 53.2793315232 +24 46 51.895675308   8.59 8.25     A5 13 0
16 HD 204843 gD* 21 30 57.0452874864 +16 34 15.570717924 8.640 8.640 8.330     A5 21 0
17 TYC 1664-433-1 SB* 21 31 01.2028669008 +16 27 40.528003896   11.67 11.27     ~ 2 0
18 TYC 2192-608-1 * 21 31 15.2223684576 +24 45 39.239017092   10.21 10.08     ~ 1 0
19 HD 207651 SB* 21 50 08.2320284304 +19 25 26.386863240   7.44 7.21     A5 30 0
20 TYC 1674-299-1 * 21 50 25.1989199064 +19 17 19.677288480   11.28 10.10     ~ 1 0
21 TYC 2758-490-1 * 22 58 13.3762757712 +33 55 04.535763420   10.85 9.50     ~ 1 0
22 HD 217241 Pu* 22 58 58.9640957040 +34 04 00.670122336   7.75 7.54     A0 12 0
23 BD+35 4999 * 23 18 29.8599457584 +36 20 32.606512872   10.90 9.53     K2 3 0
24 HD 219843 PM* 23 18 42.2618532984 +36 05 24.808875900   7.67 7.37     F0 15 0
25 BD+19 5110 * 23 28 12.3629896344 +20 00 17.280758592   10.10 9.49     G0 4 0
26 HD 221011 * 23 28 23.5397137632 +19 53 08.098418400   6.91 6.67     F0 20 0

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