A dataset provided by the European Space Agency

Name 040564
Title Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405640901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405641001

DOI 10.5270/esa-amsut7h
Author Dr Roland Walter
Description Two of the strongly absorbed super-giant HMXB discovered by INTEGRAL are eclipsing systems. This very rare property allows a comprehensive study of the dynamics and of the stellar winds in those systems. The aim of this proposal is to obtain quantitative constraints on the ionisation, density and clumping of the stellar wind along the orbit and to measure the masses of the neutron stars.
Publication 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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 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 ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 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 ,
An XMM-Newton view of FeKalpha in high-mass X-ray binaries . Gimenez-Garcia, A., Torrejon, J. M., et all. . A&A . 576-108 . 2015 . ...,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 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 ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-08-29T00:00:00Z, 040564, 17.56_20190403_1200. https://doi.org/10.5270/esa-amsut7h