TY - GEN
T1 - VSTAR models of the hot Jupiter HD 189733b
AU - Bott, Kimberly
AU - Kedziora-Chudczer, Lucyna
AU - Bailey, Jeremy
PY - 2013
Y1 - 2013
N2 - Past analysis of HD 189733b's atmosphere has been a cause for some debate, with conflicting findings regarding water and sodium abundances and the presence of a high altitude haze. We present our models of HD 189733b's atmospheric composition using VSTAR (Versatile Software for Transfer of Atmospheric Radiation). Since the effective temperature of the planet is expected to be approximately 5000K, newly available high-temperature spectral line lists were used.
AB - Past analysis of HD 189733b's atmosphere has been a cause for some debate, with conflicting findings regarding water and sodium abundances and the presence of a high altitude haze. We present our models of HD 189733b's atmospheric composition using VSTAR (Versatile Software for Transfer of Atmospheric Radiation). Since the effective temperature of the planet is expected to be approximately 5000K, newly available high-temperature spectral line lists were used.
KW - Physical data and processes: radiative transfer
KW - Planets and satellites: atmospheres
KW - Planets and satellites: composition
KW - Planets and satellites: individual: HD 189733b
UR - http://www.scopus.com/inward/record.url?scp=84891857535&partnerID=8YFLogxK
U2 - 10.1017/S1743921313008582
DO - 10.1017/S1743921313008582
M3 - Conference proceeding contribution
AN - SCOPUS:84891857535
SN - 9781107045200
VL - 8
T3 - Proceedings of the International Astronomical Union
SP - 279
EP - 280
BT - Exploring the Formation and Evolution of Planetary Systems
PB - Cambridge University Press (CUP)
ER -