2009MNRAS.398.2085S

Query : 2009MNRAS.398.2085S

2009MNRAS.398.2085S - Mon. Not. R. Astron. Soc., 398, 2085-2090 (2009/October-1)

Dynamics of possible trojan planets in binary systems.

SCHWARZ R., SULI A. and DVORAK R.

Abstract (from CDS):

This paper is devoted to the dynamical stability of possible Trojan planets in binaries and in binary systems where one of the substellar companions is not larger than a brown dwarf. Using numerical integrations, we investigated how the size of the stable region around the Lagrangian point L4depends on the mass parameter and the eccentricity of the secondary star. An additional goal of this work was to create a catalogue of all possible candidates, which could be useful for future observations to detect such objects.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): celestial mechanics

Simbad objects: 23

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Number of rows : 23
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 V* CK Cet EB* 00 22 56.9554340976 -20 39 23.657817852   10.70 10.32     A8/9V 26 0
2 CD-24 681 * 01 36 58.7669741904 -24 13 23.156239152   11.14 10.90     F0 4 0
3 HD 13189 * 02 09 40.1723129208 +32 18 59.160568824   9.04 7.55     K1II-III 88 1
4 HD 13189b Pl 02 09 40.1723129208 +32 18 59.160568824           ~ 23 1
5 * 94 Cet PM* 03 12 46.4365677072 -01 11 45.955808988   5.631 5.070     F8.5V 478 1
6 BD+57 793 * 04 21 52.7048156328 +57 49 01.889294952   10.27 9.85     F5V 170 2
7 BD+57 793b Pl 04 21 52.7048156328 +57 49 01.889294952           ~ 234 1
8 BD-13 2130 * 07 37 09.2332503816 -13 54 23.956897032   11.31 10.04     G5IV-V/K2III 78 1
9 BD-13 2130b Pl 07 37 09.2332503816 -13 54 23.956897032           ~ 21 1
10 * ksi UMa RS* 11 18 10.931880 +31 31 45.44004 4.42 4.38 3.79     F8.5:V+G2V 283 0
11 NGC 4349 127 * 12 24 35.4709473000 -61 49 11.861413644   12.85 10.82     ~ 56 1
12 NGC 4349 127b Pl 12 24 35.4709473000 -61 49 11.861413644           ~ 19 1
13 * tet Vir ** 13 09 56.9889385680 -05 32 20.414634792   4.385 4.397     A1IVs 277 0
14 HD 162020b Pl 17 50 38.3557484304 -40 19 06.072311784           ~ 60 1
15 HD 162020 * 17 50 38.3557484304 -40 19 06.072311784   10.11 9.12     K3V 158 1
16 HD 168443b Pl 18 20 03.9332862096 -09 35 44.614653900           ~ 100 1
17 HD 168443c Pl 18 20 03.9332862096 -09 35 44.614653900           ~ 96 1
18 HD 168443 PM* 18 20 03.9332862096 -09 35 44.614653900   7.62 6.92     G6V 334 1
19 CoRoT-3b Pl 19 28 13.2642131544 +00 07 18.613986132           ~ 148 1
20 CoRoT-3 EB* 19 28 13.2642131544 +00 07 18.613986132   14.199 13.292 13.099 12.54 F3V 86 1
21 * 18 Del b Pl 20 58 25.9335294984 +10 50 21.430869504           ~ 19 1
22 * 18 Del PM* 20 58 25.9335294984 +10 50 21.430869504   6.432 5.506     G6III 107 1
23 HD 223099 * 23 46 46.3634862912 -35 59 37.446853056   10.01 9.80     A2III/IV 11 0

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