The runaway O-type binary HD 14633 was likely ejected from the cluster of itsbirth by dynamical interactions in the dense environment. Recent XMM-Newtonobservations have detected a soft, nonthermal X-ray flux that likely originatesin a colliding wind shock region in the binary. The large variation in systemseparation between periastron and apastron will contribute to X-ray flux andspectral variability during the orbit. We propose observations with XMM-Newtonthat will measure the variable intra-system absorption, probe the geometry andphysical parameters of the wind shock region, and investigate abundanceanomalies in the HD 14633 binary system.
Publications
A Multiwavelength Study of the Runaway Binaries HD 14633 and HD 15137 |McSwain, M. Virginia, De Becker, Michael, et al. | BSRSL | 80-565 | 2011 | 2011BSRSL..80..565M | http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80..565M
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies |Earnshaw, H. P., Roberts, T. P., et al. | MNRAS | 483-5554 | 2019 | 2019MNRAS.483.5554E | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E
The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background |Scott Barrows, R., Comerford, Julia M., et al. | ApJ | 932-27 | 2022 | 2022ApJ...932...27S | http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S
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
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
2009-07-23T12:16:15Z/2009-07-31T13:22:54Z
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.
European Space Agency, Dr M. Virginia McSwain, 2010, 'Colliding Wind Emission in the Runaway Binary HD 14633', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2b9a964
