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| Query : 2003A&A...400..241P |
2003A&A...400..241P - Astronomy and Astrophysics, volume 400, 241-248 (2003/3-2)
Selection criteria for targets of asteroseismic campaigns.
PIJPERS F.P.
Abstract (from CDS):
Various dedicated satellite projects are underway or in advanced stages of planning to perform high-precision, long duration time series photometry of stars, with the purpose of using the frequencies of stellar oscillations to put new constraints on the internal structure of stars. It is known (cf. Brown et al., 1994ApJ...427.1013B) that the effectiveness of oscillation frequencies in constraining stellar model parameters is significantly higher if classical parameters such as effective temperature and luminosity are known with high precision. In order to optimize asteroseismic campaigns it is therefore useful to select targets from among candidates for which good spectroscopic and astrometric data already exists. This paper presents selection criteria, as well as redeterminations of stellar luminosity and reddening for stars satisfying these criteria.
Abstract Copyright: ∼
Journal keyword(s): stars: oscillations - stars: evolution - stars: fundamental parameters
Simbad objects: 41
| Number of rows : 41 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | * bet Hyi | PM* | 00 25 45.07036 | -77 15 15.2860 | 3.52 | 3.41 | 2.79 | 2.28 | 1.94 | G0V | 592 | 0 |
| 2 | * eta Cas | PM* | 00 49 06.2945942922 | +57 48 54.638239716 | 4.04 | 4.02 | 3.44 | 2.94 | 2.58 | F9V | 637 | 0 |
| 3 | * ups And | PM* | 01 36 47.8415443907 | +41 24 19.651368029 | 4.70 | 4.64 | 4.10 | 3.64 | 3.35 | F9V | 963 | 1 |
| 4 | * tau Cet | PM* | 01 44 04.0831371922 | -15 56 14.927607677 | 4.43 | 4.22 | 3.50 | 2.88 | 2.41 | G8V | 1255 | 1 |
| 5 | * alf Tri | SB* | 01 53 04.9054187154 | +29 34 43.747211027 | 3.96 | 3.90 | 3.42 | 3.00 | 2.72 | F5III | 287 | 0 |
| 6 | * tet Per | PM* | 02 44 11.9866154103 | +49 13 42.414669174 | 4.62 | 4.62 | 4.11 | 3.67 | 3.37 | F8V | 405 | 0 |
| 7 | * iot Per | PM* | 03 09 04.0193012009 | +49 36 47.802053343 | 4.76 | 4.64 | 3.7 | G0V | 548 | 0 | ||
| 8 | * alf For | PM* | 03 12 04.5298039833 | -28 59 15.439152331 | 4.41 | 4.51 | 3.98 | 3.39 | 3.08 | F6V | 272 | 0 |
| 9 | * kap01 Cet | BY* | 03 19 21.6964175772 | +03 22 12.714979884 | 5.71 | 5.52 | 4.85 | 4.27 | 3.91 | G5V | 890 | 0 |
| 10 | * eps Eri | BY* | 03 32 55.8444911587 | -09 27 29.739493865 | 5.19 | 4.61 | 3.73 | 3.00 | 2.54 | K2V | 1932 | 1 |
| 11 | * del Eri | PM* | 03 43 14.9005379551 | -09 45 48.210955899 | 5.13 | 4.46 | 3.54 | 2.82 | 2.32 | K0+IV | 598 | 0 |
| 12 | * gam Dor | gD* | 04 16 01.5866224848 | -51 29 11.932714356 | 4.55 | 4.20 | F1V | 314 | 0 | |||
| 13 | * pi.03 Ori | PM* | 04 49 50.4112051485 | +06 57 40.600622266 | 3.620 | 3.630 | 3.190 | 2.77 | 2.51 | F6V | 571 | 0 |
| 14 | * gam Lep | PM* | 05 44 27.7906169580 | -22 26 54.187756254 | 4.08 | 4.07 | 3.60 | 3.15 | 2.89 | F6V | 428 | 0 |
| 15 | * chi01 Ori | RS* | 05 54 22.9829893 | +20 16 34.222038 | 5.08 | 5.00 | 4.40 | 3.90 | 3.59 | G0V | 851 | 0 |
| 16 | * ksi Gem | PM* | 06 45 17.3644854477 | +12 53 44.141855267 | 3.85 | 3.79 | 3.36 | 2.97 | 2.74 | F5IV-V | 218 | 0 |
| 17 | * alf CMi | SB* | 07 39 18.11950 | +05 13 29.9552 | 0.82 | 0.79 | 0.37 | -0.05 | -0.28 | F5IV-V+DQZ | 1864 | 0 |
| 18 | * I Car | V* | 10 24 23.7055275402 | -74 01 53.799900604 | 4.35 | 4.36 | 4.01 | 3.67 | 3.48 | F3V | 130 | 0 |
| 19 | * iot Leo | SB* | 11 23 55.45273 | +10 31 46.2195 | 4.35 | 3.8 | F3V | 274 | 0 | |||
| 20 | * bet Vir | PM* | 11 50 41.7185158616 | +01 45 53.001539131 | 4.26 | 4.15 | 3.60 | 3.13 | 2.85 | F9V | 929 | 0 |
| 21 | * eta Boo | SB* | 13 54 41.07892 | +18 23 51.7946 | 3.440 | 3.250 | 2.680 | 2.24 | 1.95 | G0IV | 704 | 0 |
| 22 | * tet Boo | PM* | 14 25 11.7969501601 | +51 51 02.677224089 | 4.57 | 4.56 | 4.05 | 3.64 | 3.39 | F7V | 372 | 0 |
| 23 | * alf Cen B | PM* | 14 39 35.06311 | -60 50 15.0992 | 2.89 | 2.21 | 1.33 | K1V | 1024 | 2 | ||
| 24 | * alf Cen A | SB* | 14 39 36.49400 | -60 50 02.3737 | 0.96 | 0.72 | 0.01 | G2V | 1280 | 1 | ||
| 25 | * mu. Vir | PM* | 14 43 03.6239867612 | -05 39 29.524956308 | 4.25 | 4.26 | 3.88 | 3.48 | 3.26 | F2V | 227 | 0 |
| 26 | HD 140283 | Pe* | 15 43 03.0971190219 | -10 56 00.595693188 | 7.508 | 7.711 | 7.212 | 6.63 | 8.21 | F9VkA5mA1 | 937 | 0 |
| 27 | * lam Ser | PM* | 15 46 26.6142121632 | +07 21 11.047378824 | 5.13 | 5.03 | 4.42 | 3.92 | 3.60 | G0-V | 573 | 0 |
| 28 | * gam Ser | PM* | 15 56 27.1826577018 | +15 39 41.809580382 | 4.31 | 4.34 | 3.84 | 3.37 | 3.13 | F6V | 558 | 0 |
| 29 | * zet Her | SB* | 16 41 17.16104 | +31 36 09.7873 | 3.640 | 3.430 | 2.800 | 2.31 | 1.99 | G0IV | 545 | 0 |
| 30 | * 36 Oph A | PM* | 17 15 20.7836485323 | -26 36 06.117207947 | 5.93 | 5.08 | K2V | 269 | 1 | |||
| 31 | * 36 Oph | ** | 17 15 20.9839376 | -26 36 10.157115 | K2V+K1V | 136 | 0 | |||||
| 32 | * mu.01 Her | ** | 17 46 27.5472960785 | +27 43 14.560978925 | 4.56 | 4.17 | 3.42 | 2.89 | 2.51 | G5IV | 691 | 0 |
| 33 | * 70 Oph A | SB* | 18 05 27.2484131991 | +02 30 00.526614953 | 3.6 | K0V | 227 | 0 | ||||
| 34 | * chi Dra | SB* | 18 21 03.38255 | +72 43 58.2518 | 4.010 | 4.070 | 3.580 | 3.14 | 2.83 | F7V | 400 | 1 |
| 35 | * del Pav | PM* | 20 08 43.6088716052 | -66 10 55.442769229 | 4.78 | 4.32 | 3.56 | 2.95 | 2.61 | G8IV | 390 | 0 |
| 36 | * psi Cap | PM* | 20 46 05.7329952443 | -25 16 15.233491015 | 4.538 | 4.122 | F5V | 216 | 0 | |||
| 37 | * alf Oct | EB* | 21 04 43.0626765409 | -77 01 25.566080008 | 5.64 | 5.15 | F6(m)pec | 83 | 0 | |||
| 38 | * gam Pav | PM* | 21 26 26.6049826473 | -65 21 58.313057521 | 4.57 | 4.70 | 4.22 | 3.75 | 3.45 | F9VFe-1.4CH-0.7 | 411 | 0 |
| 39 | * iot Peg | SB* | 22 07 00.6655101792 | +25 20 42.356386464 | 4.190 | 4.200 | 3.770 | 3.36 | 3.11 | F5V | 443 | 1 |
| 40 | * nu. Ind | ** | 22 24 36.8853892493 | -72 15 19.488237466 | 5.94 | 5.29 | G9VFe-3.1CH-1.5 | 276 | 0 | |||
| 41 | * gam Tuc | PM* | 23 17 25.7564454336 | -58 14 08.524954176 | 4.35 | 4.37 | 3.98 | 3.57 | 3.33 | F4V | 158 | 0 |
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