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Volumn 538, Issue , 2012, Pages

Constraining the interior of extrasolar giant planets with the tidal Love number k 2 using the example of HAT-P-13b

Author keywords

methods: numerical; planets and satellites: individual: HAT P 13b; planets and satellites: interiors

Indexed keywords

ATMOSPHERE MODELS; ATMOSPHERIC CONDITIONS; DENSITY DISTRIBUTIONS; DIFFERENT BOUNDARY CONDITION; ECCENTRICITY MEASUREMENT; EXO-PLANETS; EXOPLANET; EXTERNAL BOUNDARY CONDITIONS; EXTRASOLAR GIANT PLANETS; HYDROSTATIC EQUILIBRIUM; INTERIOR STRUCTURE; ISOTHERMAL REGION; JUPITERS; LOVE NUMBERS; LOWER LIMITS; MASS CONSERVATION; METALLICITIES; METHODS: NUMERICALS; MODEL ATMOSPHERE; OUTER TEMPERATURE; PARAMETER RANGE; PLANETS AND SATELLITES: INDIVIDUAL: HAT-P-13B; RADIAL-VELOCITY OBSERVATIONS; SURFACE TEMPERATURES;

EID: 84857175278     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118141     Document Type: Article
Times cited : (52)

References (37)
  • 22
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    • 0004015797 scopus 로고
    • Physics of planetary interiors (Pachart Pub House)
    • Zharkov, V. N., & Trubitsyn, V. P. 1978, Physics of planetary interiors (Pachart Pub House), A&AS, 6
    • (1978) A&AS , pp. 6
    • Zharkov, V.N.1    Trubitsyn, V.P.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.