A dataset provided by the European Space Agency

Name: Is Nova Centauri 1986 an
Published: 2012-03-15T00:00:00Z

Proposal ID	065328
Title	Is Nova Centauri 1986 an
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653280101
DOI	https://doi.org/10.5270/esa-x2h0ch1
Principal Investigator, PI	Dr Gerardo Luna
Abstract	V842 Cen underwent a nova eruption in 1986 and in 2008 a period of 57 s has beendetected in optical photometry, likely related with the white dwarf spin makingthe system a strong candidate of the intermediate polar class. We propose to usethe unique capabilities of XMM-Newton to search for X-ray emission andcharacterize the accretion process onto the likely magnetized white dwarf.
Publications	XMM-Newton EPIC and OM observation of Nova Centauri 1986 (V842 Cen) \|Luna, G. J. M., Diaz, M. P., et al. \| MNRAS \| 423-75 \| 2012 \| 2012MNRAS.423L..75L \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423L..75L 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 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	2011-02-24T09:08:01Z/2011-02-25T00:57:42Z
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	2012-03-15T00:00:00Z
Keywords	"XMM", "nova eruption", "white dwarf spin", "optical photometry", "magnetized white dwarf", "nova centauri 1986", "XMM-Newton", "xray emission", "v842 cen", "intermediate polar class", "accretion process", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gerardo Luna, 2012, 'Is Nova Centauri 1986 an', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-x2h0ch1