A dataset provided by the European Space Agency

Name: A detailed X-ray study of the longest-lived nova in outburst, V723 Cas
Published: 2011-09-21T00:00:00Z

Proposal ID	065207
Title	A detailed X-ray study of the longest-lived nova in outburst, V723 Cas
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652070101
DOI	https://doi.org/10.5270/esa-vxorzwm
Principal Investigator, PI	Dr Jan-Uwe Ness
Abstract	With 14 years, V723Cas is the oldest nova in the Galaxy. We search for reasonsfor the long life time of this nova compared to all other novae. With anuninterrupted 60-ks XMM observation, covering one orbit, we can: (1) constrainthe location of gas in the binary system using orbit phase-resolved EPIC spectra(2) study X-ray/UV variability, yielding the WD spin period, g modeoscillations, or evidence of renewed accretion disk activity (3) seecorrelations between X-ray and UV variability (4) investigate illuminationeffects of the companion with OM (5) determine from RGS whether the X-rayspectrum is a typical SSS spectrum, or whether it consists of overlappingemission lines. (6) search for emission lines yielding information on renewed accretion and cooling ejecta
Publications	High-resolution spectroscopy and high-density monitoring in X-rays of novae \|Ness J. U. \| BASI \| 40-353 \| 2012 \| 2012BASI...40..353N \| http://ui.adsabs.harvard.edu/#abs/2012BASI...40..353N Obscuration effects in super-soft-source X-ray spectra \|Ness J.-U. Osborne J. P. et al. \| A&A \| 559-50 \| 2013 \| 2013A&A...559A..50N \| http://ui.adsabs.harvard.edu/#abs/2013A&A...559A..50N 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 Short-period X-ray oscillations in super-soft novae and persistent super-soft sources \|Ness J.-U. Beardmore A. P. et al. \| A&A \| 578-39 \| 2015 \| 2015A&A...578A..39N \| http://ui.adsabs.harvard.edu/#abs/2015A&A...578A..39N 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	2010-08-26T18:07:43Z/2010-08-27T13:00:18Z
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	2011-09-21T00:00:00Z
Last Update	2025-01-27
Keywords	"wd spin period", "mode oscillations", "binary system", "EPIC", "cooling ejecta", "renewed accretion", "uv variability", "life time", "typical sss spectrum", "v723 cas", "overlapping emission lines", "XMM", "xray spectrum", "illumination effects", "lived nova"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jan-Uwe Ness, 2011, 'A detailed X-ray study of the longest-lived nova in outburst, V723 Cas', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vxorzwm