2016ApJ...827L..17M


Query : 2016ApJ...827L..17M

2016ApJ...827L..17M - Astrophys. J., 827, L17-L17 (2016/August-2)

A planet in an 840 day orbit around a Kepler main-sequence a star found from phase modulation of its pulsations.

MURPHY S.J., BEDDING T.R. and SHIBAHASHI H.

Abstract (from CDS):

We have detected a 12 M_Jup planet orbiting in or near the habitable zone of a main-sequence A star via the pulsational phase shifts induced by orbital motion. The planet has an orbital period of 840±20 days and an eccentricity of 0.15. All known planets orbiting main-sequence A stars have been found via the transit method or by direct imaging. The absence of astrometric or radial velocity detections of planets around these hosts makes ours the first discovery using the orbital motion. It is also the first A star known to host a planet within 1σ of the habitable zone. We find evidence for planets in a large fraction of the parameter space where we are able to detect them. This supports the idea that A stars harbor high-mass planets in wide orbits.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): planets and satellites: detection - stars: oscillations - stars: variables: delta Scuti - stars: variables: delta Scuti

CDS comments: KELT-17 is BD+14 1881 in SIMBAD.

Simbad objects: 26

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Number of rows : 26
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 HD 15082 EB* 02 26 51.0582618096 +37 33 01.736482032   8.41 8.14     kA5hA8mF4 229 1
2 * bet Pic b Pl 05 47 17.0876901 -51 03 59.441135           ~ 627 1
3 BD+14 1881 Pe* 08 22 28.2046820904 +13 44 07.143774288   9.53 9.23   8.948 kA1hA5mA9Si 43 0
4 HD 95086b Pl 10 57 03.0215719872 -68 40 02.449216128           ~ 127 1
5 HD 100546b Pl 11 33 25.4408872296 -70 11 41.241297948           ~ 52 0
6 HD 131399 ** 14 54 25.30919 -34 08 34.0412   7.19 7.08 8.33   A1V 47 0
7 V* NN Ser RS* 15 52 56.1203524080 +12 54 44.429312196     16.51     DAO1+M4 287 0
8 HD 143567B LM* 16 01 55.65696 -21 58 53.0076           M8 43 0
9 BD+10 3472 ** 18 18 58.4250287592 +10 35 50.129564460   10.96 10.64   10.007 ~ 35 0
10 ASAS J190751+4629.2 dS* 19 07 50.7097759776 +46 29 11.904642240     12.610 12.74 12.165 F1V 42 0
11 BD+46 2629 ** 19 07 53.104944 +46 52 06.00420   10.12 9.70 9.80   kA2hA5mA7(IV)m: 173 0
12 Kepler-429 HS* 19 09 33.4136944848 +46 59 04.108493616           sdB 38 0
13 Kepler-1517 Em* 19 11 13.7297693304 +43 11 19.674097584   12.71 12.23     F0 38 0
14 Kepler-959 Er* 19 28 41.0829816648 +40 48 40.982271372   12.962 12.548 12.558   F5V 41 0
15 Kepler-1171 Er* 19 39 50.1408685104 +38 35 29.690504628   11.933 11.557 11.483   ~ 27 0
16 Kepler-1115 Ro* 19 39 58.0257208224 +40 08 39.826305276   11.9 11.7     A1IV 35 0
17 Kepler-516 Er* 19 42 26.1089369376 +38 44 08.674745208   12.491 12.044 11.990   ~ 35 0
18 Kepler-70 HS* 19 45 25.4745687168 +41 05 33.882248544 13.80 14.71 14.87 15.43 15.72 sdB 81 1
19 2MASS J19552513+4427104 dS* 19 55 25.1388299184 +44 27 10.454910768           A9III 12 0
20 Kepler-1648b Pl 19 57 44.3036608752 +43 37 57.478520640           ~ 2 0
21 Kepler-1648 dS* 19 57 44.3036608752 +43 37 57.478520640           F1V 16 0
22 Kepler-462b Pl 19 59 17.0778691680 +43 48 51.412412124           ~ 34 0
23 Kepler-462 Er* 19 59 17.0778691680 +43 48 51.412412124   12.074 11.738 11.616   A9V 61 0
24 V* V391 Peg HS* 22 04 12.1045050096 +26 25 07.819080600   14.41 14.61 15.00   sdB 112 2
25 * alf PsA b Pl 22 57 39.04625 -29 37 20.0533           ~ 210 1
26 * kap And B BD* 23 40 24.58 +44 20 02.8           L1 97 0

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