A dataset provided by the European Space Agency

Name: Accretion in a peculiar dwarf nova
Published: 2008-05-23T00:00:00Z

Proposal ID	040067
Title	Accretion in a peculiar dwarf nova
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400670101
DOI	https://doi.org/10.5270/esa-o0j7msh
Principal Investigator, PI	Dr Marina Orio
Abstract	We propose to observe EY Cyg, a dwarf nova that shows signatures of a past novaexplosion, an ideal target to study the physics of accretion. It is a knownX-ray source at low inclination, and a long period system, allowing a usefulcomparison with two short period novae recently observed in X-rays atquiescence, and with dwarf novae atlow inclination. EY Cyg is also one of veryfew relatively X-ray bright cataclysmic variables at quiescence, but it hasnever been observed in X-rays except for very short, mostly serendipitousexposures. We have already studied this system in great detail at ultravioletand optical wavelengths, but good quality data in the X-ray range are stillmissing.
Publications	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 X-ray properties of dwarf nova EY Cyg and the companion star using an XMM-Newton observation \|Nabizadeh Armin Balman u015eu00f6len \| AdSpR \| 66-1139 \| 2020 \| 2020AdSpR..66.1139N \| http://ui.adsabs.harvard.edu/#abs/2020AdSpR..66.1139N X-ray spectra and light curves of cooling novae and a nova like \|Sun Bangzheng Orio Marina et al. \| MNRAS \| 499-3006 \| 2020 \| 2020MNRAS.499.3006S \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.3006S 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 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 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	2007-04-23T12:43:52Z/2007-04-24T01:19:56Z
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	2008-05-23T00:00:00Z
Last Update	2025-08-04
Keywords	"low inclination", "xray range", "ey cyg", "optical wavelengths", "ideal target", "xray source", "short period novae", "quality data", "useful comparison", "dwarf nova", "period system", "past nova explosion"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marina Orio, 2008, 'Accretion in a peculiar dwarf nova', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-o0j7msh