[PDF] Top 20 New planets around three G Dwarfs
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New planets around three G Dwarfs
... six planets orbiting be- yond 4 AU are in eccentric orbits, and the sixth has giant planets in inner ...for planets be- yond 4 AU is similar to that for planets between ...in planets ... See full document
6
Three planets orbiting Wolf 1061
... The NASA Kepler mission has demonstrated that a high fraction of low-mass stars are planet hosts ( Dressing & Charbonneau 2013, 2015; Kopparapu 2013 ) , and the evidence is mounting that multi-planet systems are ... See full document
7
WASP 92b, WASP 93b and WASP 118b: three new transiting close in giant planets
... dominantly around stars brighter than ...hosting planets has enabled detailed follow up observations. The planets discovered by these surveys dominate the targets used for planetary atmo- sphere ... See full document
14
A universal spin mass relation for brown dwarfs and planets
... brown dwarfs show similarities to stars early in their lives, their spin evolutions are much more akin to those of ...measure new rotation periods for 18 young brown dwarfs in the Taurus star-forming ... See full document
10
Ionization in atmospheres of brown dwarfs and giant gas planets
... brown dwarfs and giant gas planets and a highly ionised gas in the younger brown dwarfs or ...brown dwarfs. They model the spectra of three brown dwarfs (with H α emissions) ... See full document
113
Tidal circularization of gaseous planets orbiting white dwarfs
... giant planets on more tightly packed and resonant orbits (Marois et ...of three or more plan- ets around single stars can survive the entire main se- quence and giant branch phases, only to ... See full document
15
Dust in brown dwarfs and extra solar planets VII Cloud formation in diffusive atmospheres
... a new cloud formation model by combining the cloud particle moment method of Helling & Woitke with a diffusive mixing approach, taking into account turbulent mixing and gas-kinetic diffusion for both gas and ... See full document
19
Three newly discovered sub Jupiter mass planets : WASP 69b and WASP 84b transit active K dwarfs and WASP 70Ab transits the evolved primary of a G4+K3 binary
... orbit around a relatively-young, active star, WASP-69b could be undergoing significant mass-loss due to X-ray-driven or extreme-ultraviolet-driven evaporation ... See full document
16
Cold giant planets evaporated by hot white dwarfs
... giant planets can be impeded by the presence of close and / or massive stellar ...and three short-period white dwarf plus M-dwarf ...ve new common proper motion companions using a 2 arcmin search ... See full document
9
Three low-mass planets from the Anglo-Australian planet search
... fainter dwarfs with uvby photometry suggesting metal-enrichment over solar was added in 1999 October ( Tinney et ...These dwarfs have V < 9 and were added to examine sugges- tions that metal-enriched ... See full document
9
Is it possible to detect planets around young active G and K dwarfs?
... our three- temperature model, illustrating the limb darkening in the spots and photosphere and the limb brightening in the ...centred around the V ... See full document
15
Two small temperate planets transiting nearby M dwarfs in K2 campaigns 0 and 1
... These planets along with others being discovered by K2 ( ...M dwarfs are brighter ( ...temperate planets in the mass – radius – temperature diagram, providing additional constraints on their orbital ... See full document
15
Realistic limitations of detecting planets around young active stars
... For G and K dwarfs, we find that it is possible, for models with high stellar activity and low stellar vsini, to be able to detect a 1 M J upiter mass planet within 50 epochs of observations and for the M ... See full document
6
Dust in brown dwarfs and extra solar planets IV Assessing TiO2 and SiO nucleation for cloud formation modelling
... Brown dwarfs have long been known to form dust in atmo- spheres and recent detections demonstrate their observational comparability to giant exoplanets like 2M0355 and 2M1207b (see Faherty et ... See full document
26
Orbital periods and component masses of three double white dwarfs
... white dwarfs, hence the fitted paramater values are not representative of either white dwarf com- ...the three cases and we averaged the results to obtain the final combined values of effective temperature ... See full document
8
A maximum entropy approach to detect close-in giant planets around active stars
... jupiters around extremely active stars, as long as the collected time se- ries is well adapted for DI, ...low-mass planets will be much reduced in this geometrical ... See full document
8
The chemical diversity of exo-terrestrial planetary debris around white dwarfs
... white dwarfs may vary significantly over periods that are short compared to the diffusion ...white dwarfs have no infrared excess (Farihi, Jura & Zuckerman 2009; Klein et ...white dwarfs that ... See full document
15
Dust in brown dwarfs and extrasolar planets : V Cloud formation in carbon and oxygen rich environments
... The bottom panel of Fig. 1 (left) shows that the large number of seeds in the oxygen-rich case results in the smallest average cloud particles sizes, as now more surface area is available onto which a given number of gas ... See full document
14
Spectra of Earth like planets through geological evolution around FGKM stars
... compare planets that receive the same bolomet- ric flux across different stellar hosts with atmospheric compositions and biogenic fluxes modeled after Earth’s ... See full document
16
A triple origin for the lack of tight coplanar circumbinary planets around short-period binaries
... the inner orbit eccentricity becomes highly excited, resulting in efficient shrinkage of the orbit. Interestingly, this also increases the relative strength of the torque of the outer orbit compared to the inner orbit on ... See full document
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