A dataset provided by the European Space Agency

Name: The atmospheric heating of AB Dor
Published: 2010-12-12T00:00:00Z

Proposal ID	060224
Title	The atmospheric heating of AB Dor
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602240201
DOI	https://doi.org/10.5270/esa-j8giusa
Principal Investigator, PI	Dr Uwe Wolter
Abstract	We propose simultaneous XMM-Newton/VLT-UVES observations of the bright ultrafastrotating late-type star AB Dor at X-ray, near UV and optical wavelengths. Weintend to study highly time-resolved correlations of coronal, chromospheric andphotospheric activity phenomena. AB Dor is a unique target in this contextbecause it permits an unprecedented temporal resolution, comparable tostate-of-the-art high-resolution solar spectroscopy. The requirement of strictlysimultaneous observations results from the short-lived nature of the activitysignatures under study.
Publications	X-ray activity cycle on the active ultra-fast rotator AB Doradus A?. Implication of correlated coronal and photometric variability \|Lalitha S. Schmitt J. H. M. M. \| A&A \| 559-119 \| 2013 \| 2013A&A...559A.119L \| http://ui.adsabs.harvard.edu/#abs/2013A&A...559A.119L A multi-wavelength view of AB Doradus outer atmosphere . Simultaneous X-ray and optical spectroscopy at high cadence \|Lalitha S. Fuhrmeister B. et al. \| A&A \| 560-69 \| 2013 \| 2013A&A...560A..69L \| http://ui.adsabs.harvard.edu/#abs/2013A&A...560A..69L Masses and activity of AB Doradus B a/b. The age of the AB Dor quadruple system revisited \|Wolter U. Czesla S. et al. \| A&A \| 570-95 \| 2014 \| 2014A&A...570A..95W \| http://ui.adsabs.harvard.edu/#abs/2014A&A...570A..95W 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 population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi P. Haberl F. et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M The Rotation of the Hot Gas around the Milky Way \|Hodges-Kluck Edmund J. Miller Matthew J. \| ApJ \| 822-21 \| 2016 \| 2016ApJ...822...21H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H 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 Structure and variability in the corona of the ultrafast rotator LO Pegasi \|Lalitha S. Schmitt J. H. M. M. \| A&A \| 602-26 \| 2017 \| 2017A&A...602A..26L \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A..26L Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld N. Buckley D. A. H. et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou Po-Sheng Chu You-Hua et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O Superflares on AB Doradus observed with TESS \|Schmitt J. H. M. M. Ioannidis P. et al. \| A&A \| 628-79 \| 2019 \| 2019A&A...628A..79S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..79S New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Indications of stellar coronal mass ejections through coronal dimmings \|Veronig Astrid M. Odert Petra et al. \| NatAs \| 5-697 \| 2021 \| 2021NatAs...5..697V \| http://ui.adsabs.harvard.edu/#abs/2021NatAs...5..697V AB Dor: Coronal Imaging and Activity Cycles \|Singh Gurpreet Pandey J. C. \| ApJ \| 966-86 \| 2024 \| 2024ApJ...966...86S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966...86S 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	2009-11-25T20:53:43Z/2009-11-26T13:07:45Z
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	2010-12-12T00:00:00Z
Last Update	2025-01-27
Keywords	"resolution solar spectroscopy", "vlt uves", "atmospheric heating", "xmm newton", "short lived", "XMM-Newton", "photospheric activity phenomena", "ab dor", "activity signatures", "optical wavelengths", "XMM", "time resolved correlations", "temporal resolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Uwe Wolter, 2010, 'The atmospheric heating of AB Dor', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j8giusa