A dataset provided by the European Space Agency

Name: On the stellar X-ray content of the Open Cluster Remnant NGC 1901
Published: 2010-05-27T00:00:00Z

Proposal ID	060298
Title	On the stellar X-ray content of the Open Cluster Remnant NGC 1901
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602980201
DOI	https://doi.org/10.5270/esa-yntui9t
Principal Investigator, PI	Dr Raimundo Lopes de Oliveira
Abstract	Open Cluster Remnants (OCRs) are poorly populated groups of stars in an advancedstage of the evolution of open clusters. These systems are specially rich inlate-type stars and binary systems of stars, of which a fraction is predicted bynumerical simulations and evolutionary models to be RS CVn, cataclysmicvariables and low-mass X-ray binaries. X-ray observations play an important rolefor the identification of those kinds of interacting binaries, which is crucialto validate the current models describing the final stages of star clusters. Wepropose to investigate for the first time the X-ray content of an OCR, NGC 1901,looking for signatures of accreting/interacting binary systems and active starsin order to put constraints on the evolutionary models.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi P. Haberl F. et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M 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 Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld N. Buckley D. A. H. et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou Po-Sheng Chu You-Hua et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Optical and X-Ray Studies of Marginal Contact Binary RW Dor Using TESS and XMM-Newton Observatories \|Sriram K. Mamatha Rani G. \| RAA \| 23-115020 \| 2023 \| 2023RAA....23k5020S \| http://ui.adsabs.harvard.edu/#abs/2023RAA....23k5020S 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	2009-05-16T09:04:00Z/2009-05-16T14:52:33Z
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	2010-05-27T00:00:00Z
Last Update	2025-01-27
Keywords	"numerical simulations", "cataclysmic variables", "stellar xray content", "specially rich", "evolutionary models", "models describing", "final stages", "star clusters", "xray content", "interacting binary systems", "interacting binary", "late type stars", "binary systems", "ngc 1901", "cluster remnant ocrs", "NGC 1901", "rs cvn", "advanced stage", "poorly populated", "active stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Raimundo Lopes de Oliveira, 2010, 'On the stellar X-ray content of the Open Cluster Remnant NGC 1901', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yntui9t