1999A&AS..136..419P

Query : 1999A&AS..136..419P

1999A&AS..136..419P - Astron. Astrophys., Suppl. Ser., 136, 419-420 (1999/April-2)

Evolution of the ``efficiency'' when different data sets are combined into a unified adjustment.

POURBAIX D. and EICHHORN H.

Abstract (from CDS):

Using a sample of binaries which were observed visually (VB) as well as spectroscopically for both components (SB2), we show that the efficiency almost always increases when a combined VB-SB2 solution replaces one based only on VB.

Abstract Copyright: ∼

Journal keyword(s): methods: numerical - statistical - binaries: visual - spectroscopic

Simbad objects: 37

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Number of rows : 37
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 * alf And a2* 00 08 23.25988 +29 05 25.5520 1.48 1.95 2.06 2.09 2.19 B8IV-VHgMn 479 1
2 HD 3443 SB* 00 37 20.71960 -24 46 02.1843           K1V+G 251 0
3 * eta And SB* 00 57 12.4002792266 +23 25 03.540083245 6.05 5.36 4.42 3.69 3.21 G8-III 199 0
4 HD 10009 SB* 01 37 37.7062257504 -09 24 13.759495668   6.77 6.24     F8.5VFe-0.5 125 0
5 * bet Ari SB* 01 54 38.41099 +20 48 28.9133 2.88 2.78 2.65 2.51 2.43 kA4hA5mA5Va 426 1
6 * bet Tri SB* 02 09 32.62712 +34 59 14.2694 3.26 3.14 3.00 2.86 2.78 A5III 230 0
7 * del Tri SB* 02 17 03.2303387763 +34 13 27.235383770 5.50 5.48   4.5   G0.5VFe-0.5 411 0
8 BD+42 501 SB* 02 21 03.68707 +42 46 25.2564   9.66 8.76     K0 55 0
9 * eps Cet SB* 02 39 33.7974128402 -11 52 19.551632148   5.33 4.87     F5V 215 0
10 * gam Per SB* 03 04 47.8201112829 +53 30 23.262605954 4.08 3.63 2.93 2.34 1.89 G9III+A2-III: 225 0
11 * alf Aur SB* 05 16 41.35871 +45 59 52.7693 1.33 0.88 0.08 -0.52 -0.96 G3III: 1207 0
12 * bet Aur SB* 05 59 31.7229284 +44 56 50.757259 1.97 1.93 1.90 1.82 1.83 A1IV-Vp 433 1
13 * 9 Pup ** 07 51 46.30295 -13 53 52.9169           G0V 256 0
14 * pi.01 Cnc SB* 09 12 17.5474052342 +14 59 45.776204103 7.49 7.24 6.51 5.90 5.52 G9V 234 0
15 HD 81809 ** 09 27 46.8088908054 -06 04 17.008787302           G1.5IV-V 322 0
16 * 93 Leo RS* 11 47 59.13595 +20 13 08.1500   5.07 4.52     F8III+A6III 230 1
17 * zet01 UMa SB* 13 23 55.5422805173 +54 55 31.295579890 2.11 2.271 2.220 2.10 2.12 A1.5Vas 320 0
18 * alf Cen B PM* 14 39 35.06311 -60 50 15.0992 2.89 2.21 1.33     K1V 1092 2
19 * alf Cen A SB* 14 39 36.49400 -60 50 02.3737 0.96 0.72 0.01     G2V 1352 1
20 * eta CrB ** 15 23 12.30535 +30 17 16.1701 5.60 5.56 4.98 4.50 4.22 G2V+G2V 198 0
21 HD 158614 SB* 17 30 23.79699 -01 03 46.4882 6.34     5.52   G9-IV-VHdel1 307 0
22 HD 163840 SB* 17 57 14.3391768182 +23 59 44.647993135   6.97 6.33     G2V+K2V 129 0
23 * 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
24 * chi Dra SB* 18 21 03.38255 +72 43 58.2518 4.010 4.070 3.580 3.14 2.83 F7V 420 1
25 HD 172865 ** 18 41 16.3660970 +30 17 40.672294   7.775 6.958 7.79   G5III-IV 88 0
26 HD 184467 SB* 19 31 07.9663576561 +58 35 09.604190291 7.95 7.47 6.60 6.13   K2V 170 0
27 * phi Cyg SB* 19 39 22.6059124440 +30 09 11.957279256   5.642 4.673     G8III-IV 148 0
28 HD 189340 SB* 19 59 47.2802830338 -09 57 29.634435094   6.45 5.87     F9V 170 0
29 HD 191854 SB* 20 10 13.32676 +43 56 44.0669 8.26 8.07 7.40 7.04   G4V+G8V 115 0
30 * tet Aql SB* 20 11 18.2866917111 -00 49 17.268937491 3.03 3.15 3.22 3.29 3.33 B9.5III 206 1
31 BD+40 883 SB* 21 00 05.3890094352 +40 04 12.684002015   11.588 9.969 9.63 7.96 M2.0V+M0.5V 184 0
32 * del Equ SB* 21 14 28.8153077 +10 00 25.125878 4.98 4.99 4.49 4.06 3.78 F7(V)+G0(V) 331 0
33 * ksi Cep A SB* 22 03 47.4397417176 +64 37 40.696071024   4.81 4.45 5.66   kA2.5hF2mF2(IV) 176 0
34 * ksi Cep ** 22 03 47.45499 +64 37 40.7128 4.72 4.63 4.29 3.97 3.84 Am+F7/8V 180 0
35 HD 213429 SB* 22 31 18.3282619654 -06 33 19.068890370   6.702 6.160     F8V 126 0
36 HD 214222 SB* 22 35 42.6711290705 +53 12 14.411224059 8.85 8.73 8.19 7.79   G1V 67 0
37 HD 219018 SB* 23 12 38.5914643702 +02 41 10.389669095   8.33 7.71     G5V 105 0

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