A dataset provided by the European Space Agency

Name: Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB
Published: 2008-08-29T00:00:00Z

Proposal ID	040564
Title	Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405641001
DOI	https://doi.org/10.5270/esa-amsut7h
Principal Investigator, PI	Dr Roland Walter
Abstract	Two of the strongly absorbed super-giant HMXB discovered by INTEGRAL areeclipsing systems. This very rare property allows a comprehensive study of thedynamics and of the stellar winds in those systems. The aim of this proposal isto obtain quantitative constraints on the ionisation, density and clumping ofthe stellar wind along the orbit and to measure the masses of the neutron stars.
Publications	X-ray wind tomography of the highly absorbed HMXB IGR J17252-3616 \|Manousakis A. Walter R. \| A&A \| 526-62 \| 2011 \| 2011A&A...526A..62M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..62M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia A. Torrejon J. M. et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind? \|Pradhan P. Bozzo E. \| A&A \| 610-50 \| 2018 \| 2018A&A...610A..50P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610A..50P Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM-Newton \|Aftab Nafisa Paul Biswajit \| ApJS \| 243-29 \| 2019 \| 2019ApJS..243...29A \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..243...29A Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 Common patterns in pulse profiles of high-mass X-ray binaries \|Alonso-Hernu00e1ndez J. Fu00fcrst F. et al. \| A&A \| 662-62 \| 2022 \| 2022A&A...662A..62A \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A..62A 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 Periodicity from X-ray sources within the inner Galactic disk \|Mondal Samaresh Ponti Gabriele et al. \| A&A \| 686-A125 \| 2024 \| 2024A&A...686A.125M \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A.125M 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	2006-08-29T02:33:56Z/2006-10-01T07:16:31Z
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	2008-08-29T00:00:00Z
Last Update	2025-01-27
Keywords	"absorbed hmxb", "neutron stars", "neutron star masses", "rare property allows", "stellar wind", "eclipsing systems", "stellar winds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Roland Walter, 2008, 'Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-amsut7h