Stars, planets and metals

Stars, planets and metals is …
instance of (P31):
scholarly articleQ13442814

External links are
P819ADS bibcode2003RvMP...75..101G
P356DOI10.1103/REVMODPHYS.75.101

P2093author name stringGonzalez G.
P2860cites workHelioseismologyQ21563876
The theory of brown dwarfs and extrasolar giant planetsQ21563882
A Jupiter-mass companion to a solar-type starQ29010471
Abundance Analyses of Field RV Tauri Stars. V. DS Aquarii, UY Arae, TW Camelopardalis, BT Librae, U Monocerotis, TT Ophiuchi, R Scuti, and RV TauriQ29544623
The Galactic Habitable Zone: Galactic Chemical EvolutionQ30040550
Stellar atmospheres of nearby young solar analogsQ30047437
Possible consequences of absence of "Jupiters" in planetary systemsQ33954450
Gravitational scattering as a possible origin for giant planets at small stellar distances.Q34411120
Dynamical Instabilities and the Formation of Extrasolar Planetary SystemsQ38503755
Detection of Planetary Transits Across a Sun-like StarQ54000265
The Spectroscopic Orbit of the Planetary Companion Transiting HD 209458Q54000512
The nature of super-metal-rich starsQ54012827
An Estimate of the Age Distribution of Terrestrial Planets in the Universe: Quantifying Metallicity as a Selection EffectQ55878162
The metal-rich nature of stars with planetsQ55885899
A Planet Candidate in the Stellar Triple System HD 178911Q56050782
Formation of the Giant Planets by Concurrent Accretion of Solids and GasQ56445800
Orbital migration of the planetary companion of 51 Pegasi to its present locationQ56536292
HD 80606 b, a planet on an extremely elongated orbitQ56563864
The unseen companion of HD114762: a probable brown dwarfQ56836148
Parent Stars of Extrasolar Planets. IV. 14 Herculis, HD 187123, and HD 210277Q56881771
Planetary Companions to the Metal‐rich Stars BD −10°3166 and HD 52265Q56881793
Ten Low‐Mass Companions from the Keck Precision Velocity SurveyQ56881819
A False Planet around HD 192263Q56881845
Galactic orbits of stars with planetsQ57594569
Structure and Evolution of Nearby Stars with Planets. I. Short‐Period SystemsQ57954629
Further evidence for the planet around 51 PegasiQ59052167
Evidence for planet engulfment by the star HD82943Q59052230
A search for 6Li in stars with planetsQ59246248
Derivation of the Mass Distribution of Extrasolar Planets with MAXLIMA, a Maximum Likelihood AlgorithmQ59246979
Analysis of theHipparcosObservations of the Extrasolar Planets and the Brown Dwarf CandidatesQ59246980
Luminosity-metallicity relation for stars on the lower main sequenceQ64166568
Abundances in metal-rich stars. Detailed abundance analysis of 47 G and K dwarf stars with [Me/H] > 0.10 dexQ66436201
Parent stars of extrasolar planets. V. HD 75289Q66436263
Parent stars of extrasolar planets. VI. Abundance analyses of 20 new systemsQ66436372
The abundance distribution in the extrasolar-planet host star HD 19994Q66470088
A differential spectroscopic analysis of 16 Cygni a and bQ66710331
Abundance analyses of field RV Tauri stars. IV. AD Aquilae, DS Aquarii, V360 Cygni, AC Herculis, and V453 OphiuchiQ68241028
Experimental radiative lifetimes, branching fractions, and oscillator strengths for la II and a new determination of the solar lanthanum abundanceQ68303681
Are stars with planets polluted?Q68322242
Photometric abundances for G dwarfs: a cautionary taleQ68433267
Non-interacting main-sequence binaries with different chemical compositions: Evidences of infall of rocky material?Q68509273
Giant planet formation by gravitational instabilityQ68630539
Radiative lifetimes, branching fractions and transition probabilities in Ge I - solar implicationsQ68692008
The host stars of extrasolar planets have normal lithium abundancesQ68694916
Maximum-likelihood method for estimating the mass and period distributions of extrasolar planetsQ68700057
Magnetic activity-related radial velocity variations in cool stars: first results from the Lick extrasolar planet surveyQ68798953
Nonradial oscillation in the solar-temperature star 51 PegasiQ68823160
Possible stellar metallicity enhancements from the accretion of planetsQ68823803
Solar model: Element diffusion or metal-enhanced envelope?Q68823961
Planet accretion and the abundances of lithium isotopesQ68843759
Planet consumption and stellar metallicity enhancementsQ68870657
A lack of planets in 47 Tucanae from a Hubble Space Telescope searchQ68877082
Mining the metal-rich stars for planetsQ68877218
Stellar pollution in the solar neighborhoodQ68879382
The mass of the convective zone in FGK main-sequence stars and the effect of accreted planetary material on apparent metallicity determinationsQ68879421
Eccentricity evolution of migrating planetsQ68881187
An adaptive optics search for companions to stars with planetsQ68881487
The galactic disk mass budget. II. Brown dwarf mass function and densityQ68881546
Stellar metallicity and the formation of extrasolar gas giant planetsQ68881599
A critical examination of Li pollution and giant-planet consumption by a host starQ68882361
An improved uvby-metallicity calibration for metal-rich starsQ68882985
The evolution of the lithium abundances of solar-type stars. VIII. M67 (NGC 2682)Q68921270
Production of star-grazing and star-impacting planetesimals via orbital migration of extrasolar planetsQ68921935
Planets in stellar clusters extensive search. I. Discovery of 47 low-amplitude variables in the metal-rich cluster NGC 6791 with millimagnitude image subtraction photometryQ68923554
Searching for planets in the Hyades. II. Some implications of stellar magnetic activityQ68923606
On the nature of stars with planetsQ68949840
Are stars with planets anomalous ?Q68949842
Beryllium in the Hyades F and G dwarfs from Keck HIRES spectraQ68985496
Standard Solar CompositionQ104111148
P304page(s)101–120
P577publication date2003-01-01
P1433published inReviews of Modern PhysicsQ26572
P1476titleStars, planets and metals
P478volume75

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cites work (P2860)
Q68949742Abundance ratios of volatile vs. refractory elements in planet-harbouring stars: hints of pollution?
Q68949823Effective temperatures and radii of planet-hosting stars from IR photometry
Q56144376Spectroscopic [Fe/H] for 98 extra-solar planet-host stars

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