A dataset provided by the European Space Agency

Name 060224
Title The atmospheric heating of AB Dor
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602240201

DOI 10.5270/esa-j8giusa
Author Dr Uwe Wolter
Description We propose simultaneous XMM-Newton-VLT-UVES observations of the bright ultrafast rotating late-type star AB Dor at X-ray, near UV and optical wavelengths. We intend to study highly time-resolved correlations of coronal, chromospheric and photospheric activity phenomena. AB Dor is a unique target in this context because it permits an unprecedented temporal resolution, comparable to state-of-the-art high-resolution solar spectroscopy. The requirement of strictly simultaneous observations results from the short-lived nature of the activity signatures under study.
Publication 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 ,
A multi-wavelength view of AB Doradus outer atmosphere . Simultaneous X-ray and optical spectroscopy at high cadence . Lalitha, S., Fuhrmeister, B., et all. . A&A . 560-69 . 2013 . 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 all. . A&A . 570-95 . 2014 . 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 ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 , <...
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-12-12T00:00:00Z, 060224, 17.56_20190403_1200. https://doi.org/10.5270/esa-j8giusa