A dataset provided by the European Space Agency

Name: Testing the theory of modified shocks in the wind-wind collision of HD54662
Published: 2017-10-13T22:00:00Z

Proposal ID	078015
Title	Testing the theory of modified shocks in the wind-wind collision of HD54662
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780150101
DOI	https://doi.org/10.5270/esa-w6alt9j
Principal Investigator, PI	Prof Gregor Rauw
Abstract	In an eccentric massive binary, the X-ray emission of an adiabatic windinteraction should vary as 1/d. Yet, among the few adiabatic colliding wind O +O binaries observed so far, deviations from this relation were found. Sincethese systems are non-thermal radio emitters, such deviations could reflect theimpact of modified shocks. To test this explanation, we propose to collect anX-ray spectrum of the 558 day period O-star binary HD54662 near apastron.HD54662 should feature an adiabatic wind-wind interaction, but shows no evidencefor the presence of relativistic particles. Together with an existingobservation near periastron, these data will provide a clean test of the impactof non-thermal particles on the shocks.
Publications	The long-period massive binary HD 54662 revisited \|Mossoux, E., Mahy, L., \| A&A \| 615-19 \| 2018 \| 2018A&A...615A..19M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A..19M 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	2016-09-29T05:20:29Z/2016-09-29T14:30:29Z
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	2017-10-13T22:00:00Z
Keywords	"adiabatic wind interaction", "adiabatic colliding wind", "relativistic particles", "clean test", "xray spectrum", "nonthermal radio emitters", "eccentric massive binary", "nonthermal particles", "xray emission", "modified shoc", "wind wind collision", "star binary hd54662"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Gregor Rauw, 2017, 'Testing the theory of modified shocks in the wind-wind collision of HD54662', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w6alt9j