A dataset provided by the European Space Agency

Name: First View of the Accretion Disks in Normal Symbiotic Stars
Published: 2015-11-14T23:00:00Z

Proposal ID	074061
Title	First View of the Accretion Disks in Normal Symbiotic Stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740610101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740610201
DOI	https://doi.org/10.5270/esa-gqa432k
Principal Investigator, PI	Dr Jennifer Sokoloski
Abstract	Accretion disks in symbiotic stars are often hidden by the optical emission fromthe red-giant companion, UV from the ionized nebula, and soft X-rays fromcolliding winds. A survey of symbiotic with Swift, however, has revealed thatthe accretion disk dominates above 2 keV and in the rapidly variable portion ofthe UV. To determine the basic properties of the large, wind- fed accretiondisks around the white dwarfs in symbiotic, we propose X-ray and UV observationswith XMM-Newton of the two most promising targets from our Swift survey. OnlyXMM can provide the sensitive, contiguous, multi-wavelength observations todetermine the accretion rates, characterize the properties of the UV flickeringand test our conclusion that hard X-rays originate in the innermost accretion disk.
Publications	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 An XMM-Newton View of the Symbiotic Stars HM Sge NQ Gem and PU Vul \|Toalu00e1 Jesu00fas A. Botello Marissa K. \| ApJ \| 948-14 \| 2023 \| 2023ApJ...948...14T \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...14T X-rays and TESS observations of symbiotic binary stars \|Lima I. J. Luna G. J. M. et al. \| BAAA \| 64-59 \| 2023 \| 2023BAAA...64...59L \| http://ui.adsabs.harvard.edu/#abs/2023BAAA...64...59L 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	2014-08-19T17:44:35Z/2014-10-27T06:17:37Z
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	2015-11-14T23:00:00Z
Last Update	2025-01-27
Keywords	"basic properties", "accretion disk dominates", "xmm newton", "uv flickering", "symbiotic stars", "swift survey", "hard xray", "accretion rates", "multi wavelength", "ionized nebula", "innermost accretion disk", "XMM-Newton", "soft xray", "normal symbiotic stars", "red giant companion", "white dwarfs", "promising targets", "optical emission", "XMM", "accretion dis", "colliding winds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jennifer Sokoloski, 2015, 'First View of the Accretion Disks in Normal Symbiotic Stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gqa432k