A dataset provided by the European Space Agency

Name: A Luminous Nova in Outburst
Published: 2012-12-17T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	067289
Title	A Luminous Nova in Outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672890201
DOI	https://doi.org/10.5270/esa-7tl3gy5
Principal Investigator, PI	Dr Marina Orio
Abstract	We propose to continue a program of Target of Opportunity Observations ofclassical and recurrent novae in outburst, triggered when a nova is observedwith Swift as a luminous X-ray source. Our aims are: a) to constrain the mass,temperature and chemical composition of the white dwarf by means of the RGSspectrum, b) to correlate temporal and spectral line variability during thenuclear burning phase, and c) if the shell is very X-ray bright, to use the RGSto explore also wind mass loss in a recurrent nova. The proposed study isimportant to understand the evolution of accretion and hydrogen burning on whitedwarfs in close binaries, including supernovae Ia progenitors.
Publications	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 X-Ray Grating Observations of Recurrent Nova T Pyxidis during the 2011 Outburst \|Tofflemire Benjamin M. Orio Marina et al. \| ApJ \| 779-22 \| 2013 \| 2013ApJ...779...22T \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...779...22T 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 Pre-outburst Chandra observations of the recurrent nova T Pyxidis \|Balman S. \| A&A \| 572-114 \| 2014 \| 2014A&A...572A.114B \| http://ui.adsabs.harvard.edu/#abs/2014A&A...572A.114B 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 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	2011-11-28T07:20:56Z/2011-11-28T15:56:11Z
Version	21.51_20241115_1113
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	2012-12-17T00:00:00Z
Last Update	2026-07-09
Keywords	"wind mass loss", "white dwarfs", "white dwarf", "supernova ia progenitors", "recurrent nova", "rgs spectrum", "spectral line variability", "close binary", "xray bright", "luminous nova", "chemical composition", "correlate temporal", "hydrogen burning", "nuclear burning phase", "luminous xray source", "recurrent novae"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marina Orio, 2012, 'A Luminous Nova in Outburst', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-7tl3gy5
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.