@inproceedings{455a2ed8779543bdb5125222aca8da6b,
title = "Spectroscopic characterisation of close orbiting extrasolar giant planets",
abstract = "A number of successful mid-infrared detections and studies of close orbiting extrasolar giant planetary atmospheres have been responsible for both driving and informing modelling efforts. Recent models have indicated that these planets may be subdivided into two groups, one with cooler atmospheres exhibiting solely absorption features, and a second comprising the most highly irradiated atmospheres which possess a temperature inversion leading to emission features.To date, no firm detection of the direct spectrum of a close orbiting extrasolar giant planet or “Hot Jupiter” has been made at near infrared wavelengths. We present the current status of such ground based studies of the bright systems, HD 189733 b, HD 179949 b.",
keywords = "extrasolar planets, infrared astronomy, stars",
author = "J.R. Barnes and T.S. Barman and H.R.A. Jones and C.J. Leigh and {Collier Cameron}, A. and L. Prato and R.J. Barber",
note = "“Copyright 2009 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.” [Full text of this article is not available in the UHRA]",
year = "2009",
doi = "10.1063/1.3099136",
language = "English",
isbn = "978-0-7354-0627-8",
series = "AIP Conf Procs",
publisher = "American Institute of Physics (AIP)",
pages = "417--420",
booktitle = "Cool Stars, Stellar Systems and the Sun",
address = "United States",
}