A dataset provided by the European Space Agency

Name: The Quiet HMXB Candidate HD 15137
Published: 2012-02-09T00:00:00Z

Proposal ID	065062
Title	The Quiet HMXB Candidate HD 15137
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650620201
DOI	https://doi.org/10.5270/esa-gieljsn
Principal Investigator, PI	Dr M. Virginia McSwain
Abstract	HD 15137 is an intriguing runaway O-type binary that offers a rare opportunityto explore the mechanism by which it was ejected from the open cluster of itsbirth. All of the evidence from optical spectra points to a compact companion inthis system - except for the lack of hard X-ray emission detected from thesystem. HD 15137 is therefore a quiet HMXB candidate, too widely separated forthe neutron star to accrete a significant mass of stellar winds and be detectedas an X-ray binary. Therefore we propose observations with XMM-Newton, to occurat the time of periastron, that will detect the hard power law spectrum from aweakly accreting neutron star and reveal the evolutionary history of HD 15137.
Publications	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 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 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	2011-01-23T14:53:12Z/2011-01-24T03:19:30Z
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	2012-02-09T00:00:00Z
Last Update	2025-01-27
Keywords	"hd 15137", "widely separated", "hard xray emission", "xray binary", "type binary", "xmm newton", "intriguing runaway", "compact companion", "XMM-Newton", "optical spectra", "hmxb candidate", "system except", "XMM", "neutron star", "evolutionary history", "stellar winds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr M. Virginia McSwain, 2012, 'The Quiet HMXB Candidate HD 15137', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gieljsn