A possible signature of terrestrial planet formation in the chemical composition of solar analogs

Astronomy and Astrophysics

Volumn 521, Issue 4, 2010, Pages

  Ramirez I ^a   Asplund, M ^a   Baumann, P ^a   Melendez J ^b   Bensby, T ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b CENTRO DE ASTROFÍSICA   (Portugal)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

planetary systems; Stars: abundances; Sun: abundances

Indexed keywords

CHEMICAL COMPOSITIONS; CONDENSATION TEMPERATURE; DIFFERENT ORIGINS; DWARF STARS; EARTH-LIKE PLANETS; ELEMENTAL ABUNDANCE; FIRST IONIZATION POTENTIALS; FULLY COMPATIBLE; PLANET FORMATION; PLANETARY SYSTEM; REFRACTORY ELEMENTS; STARS: ABUNDANCES; SUN: ABUNDANCES; TERRESTRIAL PLANETS;

EARTH (PLANET); GEOCHEMISTRY; IONIZATION POTENTIAL; PLANETS; SUN;

STARS;

EID: 77958024076     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014456     Document Type: Article

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