Chemical clues on the formation of planetary systems: C/O versus Mg/Si for HARPS GTO sample

Astrophysical Journal

Volumn 725, Issue 2, 2010, Pages 2349-2358

  Delgado Mena, E ^a,b   Israelian, G ^a,b   Gonzalez Hernandez J I ^a,b   Bond, J C ^c   Santos, N C ^d,e,f   Udry, S ^f   Mayor, M ^f  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

^c PLANETARY SCIENCE INSTITUTE   (United States)

^d CENTRO DE ASTROFÍSICA   (Portugal)

^e UNIVERSITY OF PORTO   (Portugal)

^f UNIVERSITÉ DE GENÈVE   (Switzerland)

Author keywords

Planetary systems; Planets and satellites:formation; Stars:abundances; Stars:atmospheres; Stars:fundamental parameters

Indexed keywords

EID: 78650135879     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/725/2/2349     Document Type: Article

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