A dataset provided by the European Space Agency

Name: The Quiet HMXB Candidates HD 14633 and HD 15137
Published: 2010-03-06T00:00:00Z

Proposal ID	055381
Title	The Quiet HMXB Candidates HD 14633 and HD 15137
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553810101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553810201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553810501
DOI	https://doi.org/10.5270/esa-5rp7ckm
Principal Investigator, PI	Dr M. Virginia McSwain
Abstract	The runaway O-type binaries HD 14633 and HD 15137 were likely ejected from thecluster of their birth by supernovae explosions in close binaries. Neither staris a known X-ray source, but they likely contain neutron stars and may be weakstellar wind accretion systems. Hence the two binaries have been classified asquiet HMXBs. We propose observations with XMM-Newton that will detect the hardpower-law spectrum from accreting or quiescent neutron star companions andreveal their evolutionary history.
Publications	Multiwavelength Observations of the Runaway Binary HD 15137 \|McSwain M. Virginia De Becker Michael et al. \| AJ \| 139-857 \| 2010 \| 2010AJ....139..857M \| http://ui.adsabs.harvard.edu/#abs/2010AJ....139..857M 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 Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-07-18T12:49:38Z/2009-01-30T05:10:46Z
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	2010-03-06T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "neutron stars", "XMM-Newton", "close binary", "quiet hmxbs ".", "xray source", "hd 15137", "xmm newton", "supernova explosions", "evolutionary history"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr M. Virginia McSwain, 2010, 'The Quiet HMXB Candidates HD 14633 and HD 15137', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5rp7ckm