A dataset provided by the European Space Agency

Name: A bright nova in outburst
Published: 2010-10-14T00:00:00Z

Proposal ID	060459
Title	A bright nova in outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604590301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604590401
DOI	https://doi.org/10.5270/esa-0oh612y
Principal Investigator, PI	Dr Marina ORIO
Abstract	We propose a TOO program to observe a classical or recurrent nova in outburst,if it is observed to turn into a luminous X-ray source with Swift. Our aims are:a) to constrain the mass, temperature and chemical composition of the whitedwarf by analyzing the spectrum, b) to correlate spectral and temporalvariability during the nuclear burning phase, and c) if the shell is very X-raybright, to use the RGS to explore wind mass loss in a recurrent nova. Theproposed study is important not only for nova/CV theory, but also forunderstanding hydrogen burning in shell in supernova Ia progenitors.
Publications	Swift X-Ray Observations of Classical Novae. II. The Super Soft Source Sample \|Schwarz Greg J. Ness Jan-Uwe et al. \| ApJS \| 197-31 \| 2011 \| 2011ApJS..197...31S \| http://ui.adsabs.harvard.edu/#abs/2011ApJS..197...31S Observations of classical and recurrent novae with X-ray gratings \|Orio M. \| BASI \| 40-333 \| 2012 \| 2012BASI...40..333O \| http://ui.adsabs.harvard.edu/#abs/2012BASI...40..333O 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 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 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 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 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 X-ray grating spectra of novae in outburst and the cases of two luminous novae in the Magellanic Clouds \|Orio Marina \| AdSpR \| 66-1193 \| 2020 \| 2020AdSpR..66.1193O \| http://ui.adsabs.harvard.edu/#abs/2020AdSpR..66.1193O 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 Nova LMC 2009a as observed with XMM-Newton compared with other novae \|Orio Marina Dobrotka Andrej et al. \| MNRAS \| 505-3113 \| 2021 \| 2021MNRAS.505.3113O \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.3113O 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	2009-08-20T14:07:47Z/2009-09-23T14:41:10Z
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	2010-10-14T00:00:00Z
Last Update	2025-01-27
Keywords	"temporal variability", "hydrogen burning", "cv theory", "chemical composition", "recurrent nova", "bright nova", "correlate spectral", "xray bright", "supernova ia progenitors", "nuclear burning phase", "white dwarf", "luminous xray source"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marina ORIO, 2010, 'A bright nova in outburst', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0oh612y