2019MNRAS.489.2069S

Query : 2019MNRAS.489.2069S

2019MNRAS.489.2069S - Mon. Not. R. Astron. Soc., 489, 2069-2078 (2019/October-3)

Lack of close-in, massive planets of main-sequence A-type stars from Kepler.

SABOTTA S., KABATH P., KORTH J., GUENTHER E.W., DUPKALA D., GRZIWA S., KLOCOVA T. and SKARKA M.

Abstract (from CDS):

Some theories of planet formation and evolution predict that intermediate-mass stars host more hot Jupiters than Sun-like stars, others reach the conclusion that such objects are very rare. By determining the frequencies of those planets we can test those theories.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - techniques: spectroscopic - stars: activity - stars: oscillations - planetary systems

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

CDS comments: p.2073: KOI-7733 not identified.

Simbad objects: 25

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Number of rows : 25
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 15082b Pl 02 26 51.0582618096 +37 33 01.736482032           ~ 403 1
2 BD+07 1721 Pe* 07 26 02.2901761080 +07 36 56.815027668   10.21 9.86     A8V+G9V/K1V 35 0
3 BD+14 1881b Pl 08 22 28.2046820904 +13 44 07.143774288           ~ 40 0
4 HD 85628b Pl 09 50 19.2009107592 -66 06 49.897904652           ~ 36 0
5 HD 133112b Pl 15 02 44.8678907928 -03 01 52.986571896           ~ 144 0
6 HD 133112 PM* 15 02 44.8678907928 -03 01 52.986571896   6.788 6.618     A4/5IV/V 86 0
7 BD+10 3472b Pl 18 18 58.4250287592 +10 35 50.129564460           ~ 33 0
8 HD 177876 EB* 19 04 04.6072024824 +48 52 00.102075096   7.80 7.68     A3IV-n 54 0
9 TYC 3541-3001-1 dS* 19 04 36.0623324904 +46 03 37.850502924   10.73 10.63     A4Vn 12 0
10 NAME BD+46 2629Ab Pl 19 07 53.1397066992 +46 52 05.922122844           ~ 181 1
11 TYC 3129-2543-1 dS* 19 13 14.2201698408 +42 54 49.553112348   11.94 11.98     A9V 8 0
12 BD+45 2925 * 19 34 46.6854222096 +45 37 11.807030640   10.34 10.17     A1V 19 0
13 HD 185603b Pl 19 38 38.7352230144 +31 13 09.217127532           ~ 184 0
14 Kepler-1115b Pl 19 39 58.0257208224 +40 08 39.826305276           ~ 17 0
15 Kepler-340b Pl 19 43 44.0327940888 +40 18 02.006070372           ~ 12 0
16 Kepler-340c Pl 19 43 44.0327940888 +40 18 02.006070372           ~ 15 0
17 HD 225570 * 19 44 01.9185476592 +38 52 58.510011216   11.23 11.25     A0V 11 0
18 HD 225856 * 19 47 47.1686670264 +40 00 57.330197352   10.123 9.906     A5IV 11 0
19 KOI-6068 EB* 19 48 43.6181540784 +45 59 18.456847332   10.65 10.41     A3V 25 0
20 HD 188874 dS* 19 55 24.3772549128 +43 29 47.941603512   10.87 10.69     A2 11 0
21 KOI-80 EB* 20 02 09.0139303296 +46 06 15.615562572   11.695 11.408 11.343   B9.5Vn 27 0
22 HD 332124b Pl 20 19 12.0048114552 +32 34 51.767012820           ~ 24 0
23 HD 195689b Pl 20 31 26.3534153736 +39 56 19.773037500           ~ 358 0
24 HD 201585b Pl 21 10 12.3723073896 +10 44 19.949472816           ~ 83 0
25 HD 201585 * 21 10 12.3723073896 +10 44 19.949472816   8.51 8.27     A8 53 0

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