A dataset provided by the European Space Agency

Name: Quiet after the storm: quiescent novae
Published: 2011-10-27T00:00:00Z

Proposal ID	065355
Title	Quiet after the storm: quiescent novae
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653550301
DOI	https://doi.org/10.5270/esa-63kopoo
Principal Investigator, PI	Dr Marina Orio
Abstract	We propose to observe five quiescent, accreting novae, 152 to 2 years after theoutburst. We will explore the role of the mass transfer rate, white dwarf massand magnetic fields in shaping the evolution and the characteristics of thethermonuclear flashes, in targets that were well monitored in outburst. Thetheory of explosive hydrogen burning in a shell on massive white dwarfs is thebasis for understanding novae and type Ia supernovae, but many observationalparameters are unknown. These observations will provide the key for betterunderstanding nova evolution. They will also be a legacy of XMM-Newton, andgroundwork for programs of future X-ray observatories.
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 A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton \|Gewering-Peine, A., Horns, D., \| JCAP \| 6-36 \| 2017 \| 2017JCAP...06..036G \| http://ui.adsabs.harvard.edu/#abs/2017JCAP...06..036G 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 Strong constraints on decay and annihilation of dark matter from heating of gas-rich dwarf galaxies \|Wadekar, Digvijay, Wang, Zihui, \| PhRvD \| 106-75007 \| 2022 \| 2022PhRvD.106g5007W \| http://ui.adsabs.harvard.edu/#abs/2022PhRvD.106g5007W 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	2010-09-30T22:15:54Z/2010-10-01T22:31:14Z
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	2011-10-27T00:00:00Z
Keywords	"mass transfer rate", "white dwarf mass", "XMM", "explosive hydrogen burning", "magnetic fields", "type ia supernova", "accreting novae", "future xray observatories", "nova evolution", "XMM-Newton", "quiescent novae", "massive white dwarfs", "thermonuclear flashes", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marina Orio, 2011, 'Quiet after the storm: quiescent novae', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-63kopoo