2010A&A...523A..15N


Query : 2010A&A...523A..15N

2010A&A...523A..15N - Astronomy and Astrophysics, volume 523, A15-15 (2010/11-2)

The HARPS search for southern extrasolar planets. XXIII. 8 planetary companions to low-activity solar-type stars.

NAEF D., MAYOR M., LO CURTO G., BOUCHY F., LOVIS C., MOUTOU C., BENZ W., PEPE F., QUELOZ D., SANTOS N.C., SEGRANSAN D., UDRY S., BONFILS X., DELFOSSE X., FORVEILLE T., HEBRARD G., MORDASINI C., PERRIER C., BOISSE I. and SOSNOWSKA D.

Abstract (from CDS):

In this paper, we present our HARPS radial-velocity data for eight low-activity solar-type stars belonging to the HARPS volume-limited sample: HD6718, HD8535, HD28254, HD290327, HD43197, HD44219, HD148156, and HD156411. Keplerian fits to these data reveal the presence of low-mass companions around these targets. With minimum masses ranging from 0.58 to 2.54MJup, these companions are in the planetary mass domain. The orbital periods of these planets range from slightly less than one to almost seven years. The eight orbits presented in this paper exhibit a wide variety of eccentricities: from 0.08 to above 0.8.

Abstract Copyright:

Journal keyword(s): planetary systems - techniques: radial velocities - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/A+A/523/A15): stars.dat hd6718.dat hd8535.dat hd28254.dat hd290327.dat hd43197.dat hd44219.dat hd148156.dat hd156411.dat>

Simbad objects: 24

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Number of rows : 24
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 HD 4113 PM* 00 43 12.5955916128 -37 58 57.477720936   8.61 7.88     G5V 96 1
2 HD 6718 PM* 01 07 48.6630425064 -08 14 01.330721808   9.087 8.45     G5V 100 1
3 HD 8535 PM* 01 23 37.2358505880 -41 16 11.279497332   8.25 7.69     G0V 71 1
4 HD 20782 PM* 03 20 03.5777546706 -28 51 14.660358176   8.03 7.38     G1.5V 203 1
5 HD 20792 * 03 20 49.8609678912 -03 06 30.045294432   8.91 7.89     K0III 14 0
6 HD 28254B PM* 04 24 50.2080139464 -50 37 20.803606572           ~ 4 0
7 HD 28254 PM* 04 24 50.7049876176 -50 37 19.882049844   8.439 7.684 8.52   G5V 58 1
8 HD 28254b Pl 04 24 50.7051607506 -50 37 19.883490178           ~ 16 1
9 HD 290327 PM* 05 23 21.5637042192 -02 16 39.433213524   9.73 8.94     G0 57 1
10 HD 43197 PM* 06 13 35.6615476152 -29 53 50.151597432   9.79 8.95     G8/K0IV/V 68 1
11 HD 44219 PM* 06 20 14.3231722488 -10 43 30.030733596   8.36 7.70     G3V 69 1
12 HD 80606 PM* 09 22 37.5768032712 +50 36 13.435326684   9.78 9.00     G8V 321 2
13 BD-08 2823 PM* 10 00 47.7204762252 -09 31 00.044866538   10.94 9.874 9.801   K4:V 70 1
14 HD 125595b Pl 14 21 23.1858379088 -40 23 38.217492873           ~ 13 1
15 HD 125595 PM* 14 21 23.1859553470 -40 23 38.220151339   10.13 9.03     K4Vk: 92 1
16 BD-07 4003 BY* 15 19 26.8269387505 -07 43 20.189497466 13.403 11.76 10.560 9.461 8.911 M3V 622 2
17 BD-07 4003e Pl 15 19 26.8271336166 -07 43 20.190958776           ~ 75 1
18 HD 148156b Pl 16 28 17.2846186438 -46 19 03.463378236           ~ 10 1
19 HD 148156 PM* 16 28 17.2846934448 -46 19 03.462605040   8.26 7.69     G0/2V 75 1
20 HD 156411b Pl 17 19 51.4003189231 -48 32 57.553800166           ~ 10 1
21 HD 156411 PM* 17 19 51.4007218944 -48 32 57.559997976   7.29 6.67     G1V(w) 77 1
22 HD 156846 PM* 17 20 34.3108875144 -19 20 01.491746388 7.20 7.10 6.52     G1V 111 1
23 * mu. Ara PM* 17 44 08.7031414872 -51 50 02.591603160   5.85 5.15     G3IV-V 524 2
24 HD 215497 PM* 22 46 36.7539769920 -56 35 58.326725148   9.92 8.95     K3V 58 1

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2023.10.03-09:24:28

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