A dataset provided by the European Space Agency

Name: X-rays and Doppler imaging: Do soft emission and accretion coincide?
Published: 2012-09-06T00:00:00Z

Proposal ID	067058
Title	X-rays and Doppler imaging: Do soft emission and accretion coincide?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670580201
DOI	https://doi.org/10.5270/esa-dcdq965
Principal Investigator, PI	Dr Uwe Wolter
Abstract	Classical T Tauri stars (CTTS) are young, accreting systems. The accretioncauses a variable soft X-ray excess and unusual line ratios in the He-liketriplets. Accretion signatures can also be seen in optical Doppler images.However, the true correlation of these different signatures only accessible bysimultaneous X-ray and ground-based observations has not been studied to date.We propose an 80 ksec XMM-Newton observation covering two full rotations of theCTTS MN Lup; furthermore, we propose simultaneous VLT/UVES spectral observationsto obtain a Doppler image of its surface. With its short rotation period andfast rotation, MN Lup is a truly unique target for these observations.
Publications	MN Lup: X-Rays from a Weakly Accreting T Tauri Star \|Gunther H. M. Wolter U. et al. \| ApJ \| 771-70 \| 2013 \| 2013ApJ...771...70G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...771...70G Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2011-08-12T00:30:17Z/2011-08-13T05:53:04Z
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	2012-09-06T00:00:00Z
Last Update	2025-01-27
Keywords	"accretion causes", "xmm newton", "line ratios", "mn lup", "XMM", "accretion signatures", "accretion coincide ?.", "uves spectral", "accreting systems", "fast rotation", "tauri stars ctts", "XMM-Newton", "short rotation period", "ctts mn lup", "optical doppler images", "doppler image", "soft emission", "x rays", "doppler imaging"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Uwe Wolter, 2012, 'X-rays and Doppler imaging: Do soft emission and accretion coincide?', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dcdq965