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HD 45364 b
Naming the Extrasolar Planets
HD45364, a Pair of Planets in a 3: 2 Mean Motion Resonance
Mètodes De Detecció I Anàlisi D'exoplanetes
Exoplanet.Eu Catalog Page 1 Star Distance Star Name Star Mass
Density Estimation for Projected Exoplanet Quantities
Survival of Exomoons Around Exoplanets 2
Characterising Exoplanets Satellite Arxiv:1310.7800V1 [Astro-Ph.IM] 29 Oct 2013
February 2019 BRAS Newsletter
Modeling Radial Velocity Data of Resonant Planets to Infer Migration Histories
Caracterizaç˜Ao Dinâmica Dos Sistemas Múltiplos De Planetas
UM ESTUDO SOBRE O Momentum ANGULAR
A New Scenario for the Origin of the 3/2 Resonant System HD 45364
President's Message
SAB C SAB 2010 ⋆ ⋆
Vol. 3 on Homogeneous Statistical Distributions Exoplanets for Their Dynamic Parameters
La Ricerca Dei Mondi Extra-Solari: Implicazioni Filosofiche Ed Aspetti Metodologici Nell’Astrofisica Moderna
DENSITY ESTIMATION for PROJECTED EXOPLANET QUANTITIES Robert A
Revised Exoplanet Radii and Habitability Using Gaia Data Release 2
Top View
XVI. HD 45364, a Pair of Planets in a 3:2 Mean Motion Resonance ,
Mass Constraints on Substellar Companion Candidates from the Re-Reduced Hipparcos Intermediate Astrometric Data
Taxonomy of the Extra-Solar Planet
![Characterising Exoplanets Satellite Arxiv:1310.7800V1 [Astro-Ph.IM] 29 Oct 2013](http://data.docslib.org/img/264x/4b66418067882841b9dc64e645f284e1.webp)
