A dataset provided by the European Space Agency

Name: MAGNETOSPHERIC INTERACTION IN THE ECCENTRIC T TAURI BINARY V1878 ORI
Published: 2017-04-29T22:00:00Z

Proposal ID	076372
Title	MAGNETOSPHERIC INTERACTION IN THE ECCENTRIC T TAURI BINARY V1878 ORI
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763720301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763720401
DOI	https://doi.org/10.5270/esa-5g1lo9u
Principal Investigator, PI	Dr Costanza Argiroffi
Abstract	We propose a coordinated X-ray, optical and mm campaign to measure the emissionduring and outside periastron for one of the brightest eccentric T Tauri binarysystems, V1878 Ori. This multiwavelength study, by probing complementarydiagnostics from different parts of the interacting stellar magnetospheres, andby enabling a direct comparison with magnetic field models, allows us tocharacterise coronal interactions during periastron passage and thusmagnetospheric interactions in PMS binaries.
Publications	The large-scale magnetic field of the eccentric pre-main-sequence binary system V1878 Ori \|Lavail A. Kochukhov O. et al. \| MNRAS \| 497-632 \| 2020 \| 2020MNRAS.497..632L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..632L Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earths Magnetosphere to the Solar Wind Proton Flux \|Zhang Yingjie Sun Tianran et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z 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 Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-03-01T13:24:20Z/2016-03-22T18:52:23Z
Version	17.56_20190403_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	2017-04-29T22:00:00Z
Last Update	2025-08-04
Keywords	"mm campaign", "magnetospheric interaction", "interacting stellar magnetospheres", "magnetic field models", "characterise coronal interactions", "magnetospheric interactions", "periastron passage", "coordinated xray", "brightest eccentric", "pms binary", "v1878 ori", "tauri binary systems", "probing complementary diagnostics"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Costanza Argiroffi, 2017, 'MAGNETOSPHERIC INTERACTION IN THE ECCENTRIC T TAURI BINARY V1878 ORI', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5g1lo9u