A dataset provided by the European Space Agency

Name: Disruption of coronal activity due to a massive hot Jupiter.
Published: 2021-05-28T00:00:00Z

Proposal ID	086156
Title	Disruption of coronal activity due to a massive hot Jupiter.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861560101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861560201
DOI	https://doi.org/10.57780/esa-ho3togq
Principal Investigator, PI	Dr Ignazio Pillitteri
Abstract	In the young system of WASP-18 the coronal emission is almost two orders ofmagnitude lower than expected for a star of its spectral type (F6) and age ( 800Myr). The puzzling behavior could be explained as due to tidal interaction withits very massive hot Jupiter (10 M J ) that prevents the formation of a magneticdynamo in the shallow convective zone of the star and of thus of the corona.Here we want to observe the system of KELT-24 which is very similar to WASP-18.It is formed by an F5 star orbited by a massive hot Jupiter every 5 days. Ameasurement of its X-ray flux and luminosity derived from a 25 ks XMM-EPICexposure can tell us if KELT-24 behaves like a young F type star of Hyades or ifits X-ray activity is quenched by the interaction with its 5 M_J hot Jupiter.
Publications	The X-ray activity of F stars with hot Jupiters: KELT-24 versus WASP-18 \|Pillitteri I. Colombo S. et al. \| A&A \| 673-61 \| 2023 \| 2023A&A...673A..61P \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..61P The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2020-05-14T19:55:06Z/2020-05-19T00:55:05Z
Version	18.02_20200221_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2021-05-28T00:00:00Z
Last Update	2025-01-27
Keywords	"tidal interaction", "spectral type f6", "EPIC", "xmm epic exposure", "magnitude lower", "f5 star orbited", "xray activity", "xray flux", "convective zone", "type star", "XMM", "coronal emission", "massive hot jupiter", "m_j hot jupiter", "magnetic dynamo", "coronal activity"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ignazio Pillitteri, 2021, 'Disruption of coronal activity due to a massive hot Jupiter.', 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-ho3togq