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| Query : 2012MNRAS.427L..21R |
2012MNRAS.427L..21R - Mon. Not. R. Astron. Soc., 427, L21-L24 (2012/November-3)
Period ratios in multiplanetary systems discovered by Kepler are consistent with planet migration.
REIN H.
Abstract (from CDS):
However, applying both stochastic and smooth migration forces to the planets simultaneously results in a period ratio distribution that is similar to the observed one. This is a natural scenario if planets form in a turbulent protoplanetary disc where these forces are always present. We show how the observed period ratio and eccentricity distribution can constrain the relative strength of these forces, a parameter which has been notoriously hard to predict for decades.
We make the source code of our simulations and the initial conditions freely available to enable the community to expand this study and include effect other than planetary migration.
Abstract Copyright: 2012 The Author Monthly Notices of the Royal Astronomical Society2012 RAS
Journal keyword(s): methods: numerical
Simbad objects: 1
| Number of rows : 1 |
| 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 |
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| 1 | BD-15 6290 | BY* | 22 53 16.7325836486 | -14 15 49.304052185 | 12.928 | 11.749 | 10.192 | 9.013 | 7.462 | M3.5V | 1106 | 1 |
| Query : 2012MNRAS.427L..21R |
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Hierarchy :
number of linked objects
whatever the membership probability is (see description here ) :
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BD-15 6290
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GSC 05819-00957
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NAME NC 59 | UBV M 5470 |
| Ci 20 1387 |
HIC 113020
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NLTT 55130
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UCAC2 26801725
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| CNS5 5644 |
HIP 113020
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8pc 212.69A |
UCAC4 379-165686
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| EPIC 206019387 | JP11 295 |
PLX 5546
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V* IL Aqr
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| EPIC 206019392 | Karmn J22532-142 | PLX 5546.00 | WEB 20121 |
| GCRV 14365 | LFT 1745 | PM J22532-1415 |
WISEA J225317.42-141556.1
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| GEN# -0.01506290 |
LHS 530
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Ross 780 | Zkh 338 |
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G 156-57A
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LPM 841 | TIC 188580272 | [RHG95] 3604 |
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G 156-57
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LTT 9244 |
TYC 5819-1255-1
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Gaia DR3 2603090003484152064
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GJ 876
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2MASS J22531672-1415489
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UBV 19209 |
Gaia DR2 2603090003484152064
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GJ 876 A
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MCC 337 | UBV 19610 |
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References (1106 between 1850 and 2026) (Total 1106)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
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