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
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	2025-01-27
Keywords	"hd 15137", "close binary", "neutron stars", "quiet hmxbs ".", "xmm newton", "xray source", "XMM-Newton", "XMM", "evolutionary history", "supernova explosions"
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