Exoplanet transmission spectroscopy: Accounting for the eccentricity and the longitude of periastron: Superwinds in the upper atmosphere of HD 209458b?

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Montalto, M ^a   Santos, N C ^a,b   Boisse, I ^a   Boue G ^a   Figueira, P ^a   Sousa, S ^a  

^a CENTRO DE ASTROFÍSICA   (Portugal)

^b UNIVERSITY OF PORTO   (Portugal)

Author keywords

planetary systems; planets and satellites: atmospheres; planets and satellites: individual: HD 209458b; techniques: spectroscopic

Indexed keywords

DIGITAL TELEVISION; ORBITAL LABORATORIES; ORBITS; PLANETS; SPECTROSCOPY; STARS; UPPER ATMOSPHERE; VELOCITY;

ATMOSPHERIC LAYERS; ATMOSPHERIC PROPERTIES; BLUE SHIFT; COMPOSITIONAL PROPERTIES; ECCENTRIC ORBITS; EXOPLANET; JUPITERS; ORBITAL ECCENTRICITY; ORBITAL PARAMETERS; PLANETARY ATMOSPHERE; PLANETARY ORBITALS; PLANETARY ORBITS; PLANETARY SURFACES; PLANETARY SYSTEM; PLANETS AND SATELLITES: ATMOSPHERES; PLANETS AND SATELLITES: INDIVIDUAL: HD 209458B; RADIAL VELOCITY; RED SHIFT; SPECTRAL LINE; STELLAR ORBITS; TECHNIQUES: SPECTROSCOPIC; TRANSMISSION SPECTROSCOPY;

SATELLITES;

EID: 79952586997     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116492     Document Type: Article

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