Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System
Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System
About this item
Full title
Author / Creator
Fossati, L , Koskinen, T , France, K , Cubillos, P E , Haswell, C A , Lanza, A F and Pillitteri, I
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
WASP-18 hosts a massive, very close-in Jupiter-like planet. Despite its young age (\(<\)1 Gyr), the star presents an anomalously low stellar activity level: the measured logR'\(_{\rm HK}\) activity parameter lies slightly below the basal level; there is no significant time-variability in the logR'\(_{\rm HK}\) value; there is no detection of the st...
Alternative Titles
Full title
Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2071672180
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071672180
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1802.00999