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| Query : 1988IAUS..132..153C |
1988IAUS..132..153C - 132nd Symposium of the IAU held in Paris, France June 29 - July 3 1987 Eds G. Cayrel de Strobel, M. Spite. The impact of very high S/N spectroscopy on stellar physics, 132, 153-161 (1988)
A method for calibrating, in absolute flux units, CA II H profiles of late type stars observed at ESO.
CASTELLI F., GOUTTEBROZE P., BECKMAN J., CRIVELLARI L. and FOING B.
Journal keyword(s):
Simbad objects: 20
| Number of rows : 20 |
| 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 | * zet Tuc | PM* | 00 20 04.2586334956 | -64 52 29.257190108 | 4.82 | 4.80 | 4.23 | 3.73 | 3.40 | F9.5V | 415 | 0 |
| 2 | * 9 Cet | BY* | 00 22 51.7884553555 | -12 12 33.969921319 | 7.29 | 7.05 | 6.39 | G2.5V | 510 | 0 | ||
| 3 | * bet Hyi | PM* | 00 25 45.07036 | -77 15 15.2860 | 3.52 | 3.41 | 2.79 | 2.28 | 1.94 | G0V | 631 | 0 |
| 4 | * tau Cet | PM* | 01 44 04.0831371922 | -15 56 14.927607677 | 4.43 | 4.22 | 3.50 | 2.88 | 2.41 | G8V | 1354 | 1 |
| 5 | * alf Hyi | PM* | 01 58 46.1385834212 | -61 34 11.359751511 | 3.33 | 3.13 | 2.84 | 2.55 | 2.39 | F0IV | 225 | 0 |
| 6 | * eps Eri | BY* | 03 32 55.8444911587 | -09 27 29.739493865 | 5.19 | 4.61 | 3.73 | 3.00 | 2.54 | K2V | 2073 | 1 |
| 7 | * alf Cen B | PM* | 14 39 35.06311 | -60 50 15.0992 | 2.89 | 2.21 | 1.33 | K1V | 1092 | 2 | ||
| 8 | * alf Cen A | SB* | 14 39 36.49400 | -60 50 02.3737 | 0.96 | 0.72 | 0.01 | G2V | 1352 | 1 | ||
| 9 | * ksi Boo | BY* | 14 51 23.37993 | +19 06 01.6994 | 5.618 | 5.370 | 4.593 | 3.91 | 3.48 | G7Ve+K5Ve | 503 | 0 |
| 10 | HD 131977 | BY* | 14 57 28.0007918772 | -21 24 55.727265310 | 7.89 | 6.83 | 5.72 | 4.74 | 4.19 | K4V | 525 | 0 |
| 11 | * bet TrA | PM* | 15 55 08.5620636 | -63 25 50.615531 | 3.19 | 3.14 | 2.85 | 2.53 | 2.38 | F1V | 174 | 0 |
| 12 | HD 147513 | PM* | 16 24 01.2911377368 | -39 11 34.729913940 | 6.17 | 6.02 | 5.376 | G5V | 389 | 1 | ||
| 13 | * zet TrA | SB* | 16 28 28.1422653048 | -70 05 03.824909916 | 5.446 | 4.899 | F9V | 226 | 0 | |||
| 14 | * gam Aps | PM* | 16 33 27.0825153352 | -78 53 49.733407072 | 4.783 | 3.854 | G8III | 102 | 0 | |||
| 15 | * 70 Oph | SB* | 18 05 27.28518 | +02 30 00.3558 | 5.40 | 4.89 | 4.03 | 3.38 | 2.92 | K0-V | 679 | 0 |
| 16 | * del Pav | PM* | 20 08 43.6088716052 | -66 10 55.442769229 | 4.78 | 4.32 | 3.56 | 2.95 | 2.61 | G8IV | 422 | 0 |
| 17 | HD 191408 | PM* | 20 11 11.9387690214 | -36 06 04.351725607 | 5.44 | 5.32 | K2.5V | 294 | 1 | |||
| 18 | HD 191408B | PM* | 20 11 12.8028949300 | -36 06 32.166102762 | M3.5 | 230 | 1 | |||||
| 19 | * bet01 Cap | SB* | 20 21 00.6665981712 | -14 46 53.067367488 | 4.14 | 3.87 | 3.08 | 2.53 | 2.03 | G9II:+B8p:Si: | 192 | 0 |
| 20 | * eps Ind | PM* | 22 03 21.6536261624 | -56 47 09.522795714 | 5.75 | 4.69 | K5V | 616 | 0 |
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