Log in to save to my catalogue

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

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071672180

Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System

About this item

Full title

Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2018-02

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

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

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

How to access this item