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	2025-08-04
Keywords	"XMM", "magnitude lower", "tidal interaction", "spectral type f6", "m_j hot jupiter", "massive hot jupiter", "f5 star orbited", "convective zone", "xray flux", "type star", "xray activity", "coronal emission", "xmm epic exposure", "magnetic dynamo", "EPIC", "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