Evidence of a massive planet candidate orbiting the young active K5V star BD+20 1790

Astronomy and Astrophysics

Volumn 512, Issue 7, 2010, Pages

  Hernan Obispo M ^a   Galvez Ortiz M C ^b   Anglada Escude G ^c,d   Kane, S R ^e   Barnes, J R ^b   De Castro, E ^a   Cornide, M ^a  

^a UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^b UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^c GEOPHYSICAL LABORATORY   (United States)

^d UNIVERSITY OF BARCELONA   (Spain)

^e NASA HEADQUARTERS   (United States)

Author keywords

Planetary systems; Stars: activity; Stars: individual BD+20 1790; Stars: late type

Indexed keywords

ASTROPHYSICS; CHROMOPHORES; ORBITS; PHOTOMETRY; SPECTROSCOPIC ANALYSIS; VANADIUM METALLOGRAPHY; VELOCITY;

HIGH RESOLUTION; MAIN SEQUENCE STARS; ORBITAL PERIODS; PLANETARY SYSTEM; ROTATIONAL VELOCITY; STARS: ACTIVITY; STARS: INDIVIDUAL; STARS:LATE TYPE;

STARS;

EID: 77951675093     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811000     Document Type: Article

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