A dataset provided by the European Space Agency

Name: V407 Cyg: A new laboratory for studying accretion and novae in symbiotic stars
Published: 2013-01-25T00:00:00Z

Proposal ID	067193
Title	V407 Cyg: A new laboratory for studying accretion and novae in symbiotic stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671930101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671930201
DOI	https://doi.org/10.5270/esa-gfhf7rc
Principal Investigator, PI	Dr Thomas Nelson
Abstract	We propose a 100 ks observation of the V407 Cyg, a symbiotic star which recentlyexperienced its first recorded nova outburst. A new X-ray observation of thesystem in quiescence will allow us to establish the timescales over whichaccretion is re-established after the nova outburst, and if it has, the rate atwhich material is accreted by the white dwarf. We will also study the long termevolution of the nova ejecta. Characterizing the accretion process andinteraction of the ejecta with the companion wind is a key part of understandingtype Ia supernovae like SN 2002ic, which exhibit evidence of strongcircumstellar interaction.
Publications	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	2011-12-29T15:07:47Z/2011-12-31T04:12:19Z
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	2013-01-25T00:00:00Z
Keywords	"circumstellar interaction", "exhibit evidence", "nova outburst", "recorded nova outburst", "symbiotic stars", "re established", "white dwarf", "v407 cyg", "term evolution", "symbiotic star", "accretion process", "companion wind", "nova ejecta"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Thomas Nelson, 2013, 'V407 Cyg: A new laboratory for studying accretion and novae in symbiotic stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gfhf7rc