A dataset provided by the European Space Agency

Name: XMM observations of Plaskett.s Star and HD159176
Published: 2005-01-01T00:00:00Z

Proposal ID	000173
Title	XMM observations of Plaskett.s Star and HD159176
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0001730601
DOI	https://doi.org/10.5270/esa-h48cyzk
Principal Investigator, PI	Dr Gregor Rauw
Abstract	We propose to gather XMM observations of two selected early-type colliding winds binaries (Plaskett.s Star & HD159176). The resultant exposures will provide high quality EPIC and RGS spectra which will be used to constrain the mass loss rates of the stars, to investigate the effects of various hydrodynamical processes and to study the chemical abundances of the stellar winds. Furthermore, the EPIC observations will enable us, for the first time, to seek for the predicted dynamical instabilities of the wind interaction region which should lead to strong variability of the X-ray flux on time scalesof 30 minutes. Our results should improve our understanding of the mass loss mechanism of massive stars and ultimately help to understand their
Publications	An XMM-Newton observation of the very young open cluster NGC 6383 \|Rauw, G., De Becker, M., et al. \| A&A \| 407-925 \| 2003 \| 2003A&A...407..925R \| http://ui.adsabs.harvard.edu/#abs/2003A&A...407..925R An XMM-Newton observation of the massive binary HD 159176 \|De Becker, M., Rauw, G., et al. \| A&A \| 416-221 \| 2004 \| 2004A&A...416..221D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...416..221D The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 3D models of radiatively driven colliding winds in massive O + O star binaries - III. Thermal X-ray emission \|Pittard, J. M., Parkin, E. R., \| MNRAS \| 403-1657 \| 2010 \| 2010MNRAS.403.1657P \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.403.1657P A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data \|Combi, J. A., Albacete-Colombo, J. F., \| A&A \| 477-125 \| 2008 \| 2008A&A...477..125C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...477..125C A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 \|Henley, David B., Shelton, Robin L., \| ApJS \| 187-388 \| 2010 \| 2010ApJS..187..388H \| http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H General X-ray properties of hot, massive stars \|Naze, Yael, \| BSRSL \| 80-109 \| 2011 \| 2011BSRSL..80..109N \| http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80..109N 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-Newton view of Plaskett.s star and its surroundings \|Linder, N., Rauw, G., et al. \| MNRAS \| 370-1623 \| 2006 \| 2006MNRAS.370.1623L \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.370.1623L Implications of the central metal abundance peak in cooling core clusters of galaxies \|Bohringer, H., Matsushita, K., et al. \| A&A \| 416-21 \| 2004 \| 2004A&A...416L..21B \| http://ui.adsabs.harvard.edu/#abs/2004A&A...416L..21B 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 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 An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze, Y., \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D Discovery of a magnetic field in the rapidly rotating O-type secondary of the colliding-wind binary HD 47129 (Plaskett.s star) \|Grunhut, J. H., Wade, G. A., et al. \| MNRAS \| 428-1686 \| 2013 \| 2013MNRAS.428.1686G \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.428.1686G X-Ray Observation of the Galactic Supernova Remnant G355.6-0.0 with Suzaku \|Minami, Sari, Ota, Naomi, et al. \| PASJ \| 65-99 \| 2013 \| 2013PASJ...65...99M \| http://ui.adsabs.harvard.edu/#abs/2013PASJ...65...99M 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 X-Ray Emission from Magnetic Massive Stars \|Naze, Yael, Petit, Veronique, et al. \| ApJS \| 215-10 \| 2014 \| 2014ApJS..215...10N \| http://ui.adsabs.harvard.edu/#abs/2014ApJS..215...10N Cosmology with galaxy clusters in the XMM large-scale structure survey \|Refregier, A., Valtchanov, I., \| A&A \| 390-1 \| 2002 \| 2002A&A...390....1R \| http://ui.adsabs.harvard.edu/#abs/2002A&A...390....1R Sunyaev-Zel.dovich 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 Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Is the Pollock.s paradigm of X-ray emission for O stars correct? \|Ryspaeva, E. B., Kholtygin, A. F., \| AN \| 338-959 \| 2017 \| 2017AN....338..959R \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..959R 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 Analysis of the X-ray emission of OB stars: O stars \|Ryspaeva, Elizaveta, Kholtygin, Alexander, \| RAA \| 18-104 \| 2018 \| 2018RAA....18..104R \| http://ui.adsabs.harvard.edu/#abs/2018RAA....18..104R The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H CIELO-RGS: a catalog of soft X-ray ionized emission lines \|Mao, Junjie, Kaastra, Jelle S., et al. \| A&A \| 625-122 \| 2019 \| 2019A&A...625A.122M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A.122M 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 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 An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data \|Anastasopoulou, K., Ponti, G., et al. \| A&A \| 671-55 \| 2023 \| 2023A&A...671A..55A \| http://ui.adsabs.harvard.edu/#abs/2023A&A...671A..55A 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	2001-03-09T09:41:25Z/2003-03-16T22:06:14Z
Version	PPS_NOT_AVAILABLE
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	2005-01-01T00:00:00Z
Keywords	"mass loss rates", "XMM", "stellar winds", "predicted dynamical instabilities", "xray flux", "hydrodynamical processes", "time scales", "massive stars", "quality epic", "HD159176", "EPIC", "chemical abundance", "rgs spectra", "mass loss mechanism", "wind interaction region"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gregor Rauw, 2005, 'XMM observations of Plaskett.s Star and HD159176', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-h48cyzk