2010ApJ...710.1365B


Query : 2010ApJ...710.1365B

2010ApJ...710.1365B - Astrophys. J., 710, 1365-1374 (2010/February-3)

Angular diameters and effective temperatures of 25 K giant stars from the CHARA array.

BAINES E.K., DOLLINGER M.P., CUSANO F., GUENTHER E.W., HATZES A.P., McALISTER H.A., TEN BRUMMELAAR T.A., TURNER N.H., STURMANN J., STURMANN L., GOLDFINGER P.J., FARRINGTON C.D. and RIDGWAY S.T.

Abstract (from CDS):

Using Georgia State University's Center for High Angular Resolution Astronomy Array interferometer, we measured angular diameters for 25 giant stars, six of which host exoplanets. The combination of these measurements and Hipparcos parallaxes produces physical linear radii for the sample. Except for two outliers, our values match angular diameters and physical radii estimated using photometric methods to within the associated errors with the advantage that our uncertainties are significantly lower. We also calculated the effective temperatures for the stars using the newly measured diameters. Our values do not match those derived from spectroscopic observations as well, perhaps due to the inherent properties of the methods used or because of a missing source of extinction in the stellar models that would affect the spectroscopic temperatures.

Abstract Copyright:

Journal keyword(s): infrared: stars - planetary systems - stars: fundamental parameters - techniques: interferometric - techniques: spectroscopic

Simbad objects: 49

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Number of rows : 49
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 Cl Melotte 25 OpC 04 29 47.3 +16 56 53           ~ 3074 0
2 HD 31675 PM* 05 02 50.4383043673 +66 49 22.701831787   6.67   5.9   F6V: 46 0
3 HD 32518 PM* 05 09 36.7203662520 +69 38 21.854780160 8.550 7.530 6.420     K1III 56 1
4 HD 60294 * 07 36 47.0350608048 +55 45 18.225179028   7.056 5.931     K2III 41 0
5 HD 63332 PM* 07 51 05.7111574560 +54 07 45.268427460   6.493 6.020     F6V 65 0
6 * 30 Lyn PM* 08 20 26.0598825840 +57 44 35.806402284   6.272 5.877     F4V 61 0
7 * pi.02 UMa PM* 08 40 12.8171670288 +64 19 40.570243212 6.94 5.78 4.61 3.72 3.09 K1+III 165 1
8 HD 98673 PM* 11 21 49.2888601392 +57 04 29.481890016 6.680 6.600 6.440   6.25 A7Vn 51 0
9 HD 102328 * 11 46 55.6222860288 +55 37 41.480416020   6.528 5.254     K2.5IIIbCN1 158 0
10 * 66 UMa * 11 55 58.4171473200 +56 35 54.807896544   6.928 5.824     K1III 59 0
11 HD 106574 * 12 15 08.4919348200 +70 12 00.030617424   6.909 5.719     K2III 36 0
12 HD 107193 * 12 18 49.9851888120 +75 09 38.018570112   5.504 5.460     A1V 54 0
13 HD 108954 PM* 12 30 50.1358011744 +53 04 35.784940872       5.9   F9V 128 0
14 HD 113049 * 12 58 47.3396746248 +75 28 21.079377696   7.027 5.990     K0III 40 0
15 HD 118904 * 13 37 10.9876472376 +71 14 32.097528276   6.711 5.496     K2III 42 0
16 * 3 UMi PM* 14 06 56.3646413832 +74 35 37.618422360 6.700 6.580 6.440     A7V 28 0
17 HD 132254 PM* 14 56 23.0403907176 +49 37 42.419704116   6.13   5.3   F8-V 137 0
18 * 11 UMi * 15 17 05.8894632720 +71 49 26.047336872   6.384 5.015     K4III 123 1
19 HD 137443 PM* 15 22 38.4084286968 +63 20 29.274668484   7.039 5.712     K4III 38 0
20 HD 138265 * 15 27 51.4237531200 +60 40 12.796947012 9.030 7.350 5.900     K5III 40 0
21 HD 139357 * 15 35 16.1985929736 +53 55 19.709392008   7.160 5.964     K4III: 63 1
22 HD 145454 PM* 16 06 19.6767729888 +67 48 36.486764388   5.407 5.441     A0Vn 55 0
23 HD 149681 PM* 16 25 43.1853867312 +78 57 49.885598988 5.870 5.800   5.4   F0V 37 0
24 HD 150010 PM* 16 31 28.2272499978 +72 36 44.417039002   7.64 6.31     K2III 35 0
25 HD 149303 * 16 31 47.2275879216 +45 35 53.744910612 5.850 5.78 5.68 7.16   A2Vn_lB 63 0
26 HD 151044 PM* 16 42 27.8123142480 +49 56 11.181141888       6.2   F8V 131 0
27 HD 152812 SB* 16 53 17.5500684960 +47 25 00.163611660   7.300 5.987     K2III 49 0
28 HD 157681 * 17 21 45.3683593608 +53 25 13.548351756   7.147 5.677     K4III 49 0
29 HD 158460 * 17 25 41.3535370032 +60 02 54.233277972   5.666 5.645     A1Vn 51 0
30 * x Her * 17 26 44.2419822528 +48 15 36.221599656 6.080 5.960 5.830     A4V 64 0
31 * y Her PM* 17 36 37.6537001976 +48 35 08.277294480   6.503 5.353     K1III 50 0
32 HD 161693 * 17 43 59.1688824432 +53 48 06.146004348 5.780 5.770 5.760     A2V 57 0
33 HD 167042 PM* 18 10 31.6398993768 +54 17 11.592196980   6.89   5.4   K1III 154 1
34 * 42 Dra PM* 18 25 59.1369601368 +65 33 48.531343788   6.005 4.823     K1.5IIIFe-1 167 1
35 HD 172569 PM* 18 36 13.2672431064 +65 29 19.336764120 6.440 6.340 6.060     F0V 50 0
36 HD 172728 PM* 18 37 33.5174187456 +62 31 35.673279564 5.530 5.690 5.740     A0V 78 0
37 HD 175823 * 18 53 46.3094101968 +57 29 11.606081532   7.483 6.232     K5III: 29 0
38 * 48 Dra PM* 18 56 45.0357338352 +57 48 53.339590224   6.835 5.663     K1III 55 0
39 * 51 Dra * 19 04 55.1654401944 +53 23 47.960875608   5.37 5.38     A0Vn 58 0
40 HD 184960 PM* 19 34 19.7892769104 +51 14 11.827409604   6.21   5.4   F7V 155 0
41 HD 186760 PM* 19 43 14.4186159816 +58 00 59.821870032   6.871 6.295     G0V 71 0
42 HD 186815 * 19 43 39.4962813072 +57 02 33.777357000   7.179 6.282     K2III 34 0
43 HD 188793 PM* 19 53 35.4285483408 +59 42 31.169293848   6.084 6.058     A3V 32 0
44 HD 192781 PM* 20 13 27.6162878448 +60 38 26.050279164   7.281 5.780     K5III 43 0
45 HD 195820 PM* 20 31 21.1513761912 +52 18 34.284100680   7.238 6.207     K0III 42 0
46 * 4 Cep * 20 43 11.0211392808 +66 39 26.810352432 5.880 5.810 5.600     A8V 56 0
47 HD 200205 * 20 59 25.3846975896 +59 26 18.960547380   6.942 5.526     K4III 48 0
48 HD 211211 PM* 22 14 44.3613363960 +42 57 14.038829388 5.680 5.720 5.720     A2Vnn 55 0
49 * 11 Lac PM* 22 40 30.8584750462 +44 16 34.706857320 7.15 5.79 4.46 3.54 2.86 K2.5III 138 0

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