A dataset provided by the European Space Agency

Name: Unveil accretion onset mechanisms of a normal outburst of EXO 2030+375
Published: 2015-09-22T22:00:00Z

Proposal ID	074524
Title	Unveil accretion onset mechanisms of a normal outburst of EXO 2030+375
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745240201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745240301
DOI	https://doi.org/10.5270/esa-me3lgg4
Principal Investigator, PI	Dr Carlo Ferrigno
Abstract	We propose to observe the Be/X-ray binary system EXO 2030+375 during itsperiastron passage for 30 ks to study the onset of the accretion activity.Accretion disc instability at the border of the magnetosphere have beenevidenced by quasi-periodic hour-long flux oscillations detected during INTEGRALserendipitous observations in 2011 and by EXOSAT in 1985. Existing RXTEsnapshots observations during past outbursts are unable to characterise the wayin which matter begins to penetrate into the magnetosphere. The unprecedentedsensitivity of XMM-Newton and its continuous coverage will allow us toinvestigate in detail the opening of the magnetic gate for this high-magneticfield neutron star.
Publications	Glancing through the accretion column of EXO 2030+375 \|Ferrigno Carlo Pjanka Patryk et al. \| A&A \| 593-105 \| 2016 \| 2016A&A...593A.105F \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A.105F 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 Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars \|Manikantan Hemanth Paul Biswajit et al. \| MNRAS \| 531-530 \| 2024 \| 2024MNRAS.531..530M \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..530M 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	2014-05-29T23:01:34Z/2014-05-30T10:21:49Z
Version	PPS_NOT_AVAILABLE
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	2015-09-22T22:00:00Z
Last Update	2025-01-27
Keywords	"existing rxte snapshots", "exo 2030", "quasi periodic", "xmm newton", "magnetic gate", "XMM-Newton", "accretion disc instability", "periastron passage", "past outburst", "flux oscillations", "XMM", "continuous coverage", "accretion activity", "normal outburst"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Carlo Ferrigno, 2015, 'Unveil accretion onset mechanisms of a normal outburst of EXO 2030+375', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-me3lgg4