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Searching for a gas cloud surrounding the WASP-18 planetary system

Fossati, Luca; Ayres, T. R.; Haswell, C. A.; Jenkins, J. S.; Bisikalo, D.; Bohlender, D.; Flöer, L. and Kochukhov, O. (2014). Searching for a gas cloud surrounding the WASP-18 planetary system. Astrophysics and Space Science, 354(1) pp. 21–28.

DOI (Digital Object Identifier) Link: https://doi.org/10.1007/s10509-014-2016-6
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Abstract

Near-UV (NUV) Hubble Space Telescope (HST) observations of the extreme hot-Jupiter WASP-12b revealed the presence of diffuse exospheric gas extending beyond the planet's Roche lobe. Furthermore the NUV observations showed a complete lack of the normally bright core emission of the Mg ii h&k resonance lines, in agreement with the measured anomalously low stellar activity index (logR' HK). Comparisons with other distant and inactive stars, and the analysis of radio and optical measurements of the intervening interstellar medium (ISM), led us to the conclusion that the system is surrounded by a circumstellar gas cloud, likely formed of material lost by the planet. Similar anomalous (logR' HK) index deficiencies might therefore signal the presence of translucent circumstellar gas around other stars hosting evaporating planets; we identified five such systems and WASP-18 is one of them. Both radio and optical observations of the region surrounding WASP-18 point towards a negligible ISM absorption along the WASP-18 line of sight. Excluding the unlikely possibility of an intrinsic anomalously low stellar activity, we conclude that the system is probably surrounded by a circumstellar gas cloud, presumably formed of material lost by the planet. Nevertheless only a far-UV spectrum of the star would provide a definite answer. Theoretical modelling suggests WASP-18b undergoes negligible mass loss, in contrast to the probable presence of a circumstellar gas cloud formed of material lost by the planet. The solution might be the presence either of an extra energy source driving mass loss (e.g., the reconnection of the stellar and planetary magnetic fields inside the planet atmosphere) or of an evaporating third body (e.g., moon).

Item Type: Journal Item
Copyright Holders: 2014 Springer
ISSN: 1572-946X
Keywords: Stars: individual (WASP-12, WASP-18); Planets and satellites: individual (WASP-12, WASP-18); Planet-star interactions
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 46922
Depositing User: Carole Haswell
Date Deposited: 02 Aug 2016 15:35
Last Modified: 07 Dec 2018 10:43
URI: http://oro.open.ac.uk/id/eprint/46922
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