The HARPS search for southern extra-solar planets: XXVIII. Up to seven planets orbiting HD 10180: Probing the architecture of low-mass planetary systems

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Lovis, C ^a   Segransan D ^a   Mayor, M ^a   Udry, S ^a   Benz, W ^b   Bertaux, J L ^c   Bouchy, F ^d,e   Correia, A C M ^f   Laskar, J ^g   Lo Curto, G ^h   Mordasini, C ^b,i   Pepe, F ^a   Queloz, D ^a   Santos, N C ^a,j  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b UNIVERSITY OF BERN   (Switzerland)

^c LABORATOIRE DES SCIENCES DU CLIMAT ET DE L ENVIRONNEMENT   (France)

^d INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^e OBSERVATOIRE DE HAUTE PROVENCE   (France)

^f UNIVERSITY OF AVEIRO   (Portugal)

^g Institut de Mecanique Celeste et de Calcul des ephemerides   (France)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^j UNIVERSITY OF PORTO   (Portugal)

more..

Author keywords

planets and satellites: detection; stars: individual: HD 10180; techniques: radial velocities; techniques: spectroscopic

Indexed keywords

DYNAMICAL STABILITY; EXTRA SOLAR PLANETS; GAS GIANT; GENERAL RELATIVITY; HIGH-PRECISION; ICE GIANTS; INTEGER VALUES; LOGARITHMIC SCALE; LOW-MASS; LOW-MASS SYSTEMS; MASSIVE SYSTEMS; METAL-RICH STARS; METALLICITIES; MINIMUM MASS; MOTION RESONANCES; NEPTUNE; NEW HIGH; NONRESONANT; NUMERICAL INTEGRATIONS; ORBITAL ARCHITECTURE; ORBITAL PERIODS; PLANET FORMATION; PLANETARY SYSTEM; PLANETS AND SATELLITES; PROTOPLANETS; RADIAL VELOCITY; SOLAR TYPE STARS; STARS: INDIVIDUAL: HD 10180; TECHNIQUES: RADIAL VELOCITIES; TECHNIQUES: SPECTROSCOPIC; TIDAL DISSIPATION;

ARCHITECTURE; OPTIMIZATION; PLANETS; RELATIVITY; STABILITY; STARS; SURVEYS; VELOCITY;

SATELLITES;

EID: 79952607204     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015577     Document Type: Article

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