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Be 7 solar neutrino measurement with KamLANDCurrent Status and Future Prospects of the SNO+ ExperimentInterferometric observations of rapidly rotating starsThe millimeter IRAM-30 m line survey toward IK TauExoplanetary Atmospheres-Chemistry, Formation Conditions, and HabitabilityThe frequency of planetary debris around young white dwarfsThe metallicity signature of evolved stars with planetsA high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formationAges and fundamental properties of Kepler exoplanet host stars from asteroseismologyFundamental properties of nearby single early B-type starsFundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before deathChandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rateHD 66051, an eclipsing binary hosting a highly peculiar, HgMn-related starRR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system.Disk evolution, element abundances and cloud properties of young gas giant planets.Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud.A single low-energy, iron-poor supernova as the source of metals in the star SMSS J031300.36-670839.3.Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way.R-process enrichment from a single event in an ancient dwarf galaxy.Early inner solar system origin for anomalous sulfur isotopes in differentiated protoplanets.Synthesis of refractory organic matter in the ionized gas phase of the solar nebulaA study of the dissociative recombination of CaO+ with electrons: Implications for Ca chemistry in the upper atmosphere.Silicon chemistry in the mesosphere and lower thermosphere.Evidence from stable isotopes and (10)Be for solar system formation triggered by a low-mass supernova.Carbon monoxide in an extremely metal-poor galaxy.Pure iron grains are rare in the universeALMA detection and astrobiological potential of vinyl cyanide on Titan.Carbon monoxide in clouds at low metallicity in the dwarf irregular galaxy WLM.Sources of cosmic dust in the Earth's atmosphereAstrochemistry of dust, ice and gas: introduction and overview.The origin of inner Solar System water.General active space commutator-based coupled cluster theory of general excitation rank for electronically excited states: implementation and application to ScH.[C ii] 158-μm emission from the host galaxies of damped Lyman-alpha systems.Peering through Jupiter's clouds with radio spectral imaging.Communication: The formation of CHe(2+) by radiative association.Chemical complexity in the horsehead photodissociation region.Hydrogen Bonds and Life in the Universe.Collisional excitation of interstellar PO(X2Π) by He: new ab initio potential energy surfaces and scattering calculations.Interacting supernovae from photoionization-confined shells around red supergiant stars.Large Enhancement in High-Energy Photoionization of Fe XVII and Missing Continuum Plasma Opacity.
P2860
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P2860
description
article
@en
im September 2009 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2009
@uk
ലേഖനം
@ml
name
The Chemical Composition of the Sun
@en
The Chemical Composition of the Sun
@nl
type
label
The Chemical Composition of the Sun
@en
The Chemical Composition of the Sun
@nl
prefLabel
The Chemical Composition of the Sun
@en
The Chemical Composition of the Sun
@nl
P1476
The Chemical Composition of the Sun
@en
P2093
A. Jacques Sauval
Nicolas Grevesse
P304
P356
10.1146/ANNUREV.ASTRO.46.060407.145222
P407
P577
2009-09-01T00:00:00Z