[PDF] Top 20 Star-planet interactions and dynamical evolution of exoplanetary systems
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Star-planet interactions and dynamical evolution of exoplanetary systems
... the planet-formation process. Tidal interactions cause the evolution of their orbital parameters on secular time-scales and shape their observed ...the star through magnetic ...of ... See full document
7
Stellar magnetic activity – Star-Planet Interactions
... exoplanetary systems. The activity-induced high-energy emission of the host star can influence exoplanetary atmospheres through stellar flares and can cause atmospheric ...through ... See full document
6
A long-period planet orbiting a nearby Sun-like star
... At a distance of 22 pc, HD 134987 is one of the more nearby exoplanetary systems. The com- bination of the close distance and long period indicates a relatively large angular distance from the star ... See full document
31
Monte Carlo Simulations of Stellar Planet Capture and Orbital Perturbations in Rogue Star – Solar System Interactions
... The dynamical evolution of the Solar System was determined using a numerical analysis algorithm with small time increments of 600 ...rogue star influencing their ... See full document
12
A gap in the mass distribution for warm Neptune and terrestrial planets
... the planet distribution provides an insight into the processes that shape the formation and evolution of ...the planet population for sub-Neptune-mass planets with orbital periods less than 20 ...the ... See full document
6
Relating binary star planetary systems to central configurations
... Binary-star exoplanetary systems are now known to be common, for both wide and close ...orbital evolution is generally ...include dynamical architec- tures known as central ...planetary ... See full document
10
Detection and Characterization of Extrasolar Planets through Planet-Disk Dynamical Interactions
... a planet are smeared out by collisional interactions of the dust ...dust-poor systems exist, and it is to those that we turn our attention ... See full document
171
Wobbling ancient binaries - here be planets?
... two systems, NN Ser and UZ For, our dynamical simulations reveal that the candidate companions would move on orbits that are stable on long ...those systems cannot be ruled out on the basis of their ... See full document
14
Tidal dissipation in stars and fluid planetary layers and its impact on the evolution of star-planet systems
... The properties of fluid tidal dissipation have a direct impact on the secular dynamics of planetary sys- tems. Indeed, dissipation resonances cause local rapid changes of orbital parameters, that are directly related to ... See full document
5
The dynamical fate of self gravitating disc fragments after tidal downsizing
... of planet/brown dwarf formation proposes that protostellar discs can fragment into objects with masses above a few Jupiter masses at large semimajor ...parent star-forming ...subsequent dynamical ... See full document
10
Properties of the single Jovian planet population and the pursuit of solar system analogues
... the dynamical evolution of the system, and what impact that may have had on the ...a planet to avoid being removed from a system (by collision or ejection) and remain within the ...the ... See full document
13
Tidal instability in exoplanetary systems evolution
... the evolution of extrasolar planetary systems: the tidal (or elliptical) ...hot-jupiter systems, when the rota- tion period of the star is ...dozen systems, summarized in the form of a ... See full document
7
The Pan-Pacific planet search. VII. The most eccentric planet orbiting a giant star
... put in the queue to catch the next predicted large velocity excursion of 2015 October. We were fortunate to catch the peak and the drop-off, con fi rming the period at 415 days. FEROS observations were also added and ... See full document
13
The dynamical evolution of dwarf planet (136108) Haumea's collisional family: general properties and implications for the trans-Neptunian belt
... the dynamical transfer of theoretical family escapees on to cometary ...typical dynamical lifetime of short-period comets with esti- mated lifetimes typically of the order of 10 4 –10 5 years ... See full document
20
The Interplay of Order and Disorder in the Dynamical Evolution of Physical and Biological Systems
... Conflicts of Interest: The authors declare no conflict of interest. A brief history of the multiverse. Inflationary spacetimes are not past-complete. The Entropy of the Universe and [r] ... See full document
14
Meinongian Semantics for Propositional Semantic Networks
... A SNePS representation o£ "l'he Morning Star is the Evening Star' m6 and 'The Morning Star is a planet' m9 on Castaneda's theory.. Ileum, el`and fed.!, Mind Design: I'hiJo~ophy I'sychob~[r] ... See full document
6
Derivation of the parameters of CoRoT planets
... as systems instead of separate objects, and a careful understanding of the observational and theoretical uncertainties (see in particular Sections 3 and ... See full document
7
Young brown dwarfs and their environments : testing star and planet formation
... illu strate d in Fig 1.2, w here th e tracks shown are ad ap ted from th e works of Iben (1965); H ayashi (1970); D ’A ntona &: M azzitelli (1985); C habrier &: Baraffe (2000); Siess et al. (2000), such stars ... See full document
163
Studying young stellar objects with near-IR non-redundant aperture masking and millimeter interferometry
... triggering star formation by perturbing other regions of the same cloud, which leads to the formation of multiple stars instead of a single one (Federrath et ... See full document
288
The debris disc of solar analogue tau Ceti : Herschel observations and dynamical simulations of the proposed multiplanet system
... additional planet candidates are ruled out (white area) has been estimated by assuming there is an additional planet with a semi-major axis in ex- cess of those of the previously proposed ...sixth ... See full document
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