A dataset provided by the European Space Agency

Name: High Resolution X-ray Spectroscopy of Zeta Puppis
Published: 2001-12-29T00:00:00Z

Proposal ID	009581
Title	High Resolution X-ray Spectroscopy of Zeta Puppis
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095810401
DOI	https://doi.org/10.5270/esa-qotn320
Principal Investigator, PI	Dr Albert Brinkman
Abstract	Zeta Pup is the prototypical star for studies of winds in hot stars. It shows rotationally modulated variations in both the total flux and lin widthspresumably due to inhomogeneities on the stellar surface and in the atmosphericdensities, and intrinsic instabilities in the wind structure. We will observeZeta Pup during the PV program in order to test the RGS capability to resolvevelocity fields and bulk motion.
Publications	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 A detailed X-ray investigation of zeta Puppis. I. The dataset and some preliminary results \|Naze Y. Flores C. A. \| A&A \| 538-22 \| 2012 \| 2012A&A...538A..22N \| http://ui.adsabs.harvard.edu/#abs/2012A&A...538A..22N 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 High resolution X-ray spectroscopy of zeta Puppis with the XMM-Newton reflection grating spectrometer \|Kahn S. M. Leutenegger M. A. et al. \| A&A \| 365-312 \| 2001 \| 2001A&A...365L.312K \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.312K Evidence for micrometeoroid damage in the pn-CCD camera system aboard XMM-Newton \|Struder L. Aschenbach B. et al. \| A&A \| 375-5 \| 2001 \| 2001A&A...375L...5S \| http://ui.adsabs.harvard.edu/#abs/2001A&A...375L...5S Evidence for the Importance of Resonance Scattering in X-Ray Emission Line Profiles of the O Star zeta Puppis \|Leutenegger Maurice A. Owocki Stanley P. et al. \| ApJ \| 659-642 \| 2007 \| 2007ApJ...659..642L \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...659..642L 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 X-ray spectroscopy of early-type stars: The present and the future \|Rauw G. Naze Y. \| AN \| 329-222 \| 2008 \| 2008AN....329..222R \| http://ui.adsabs.harvard.edu/#abs/2008AN....329..222R X-rays clumping and wind structures \|Oskinova Lidia Hamann Wolf-Rainer et al. \| BSRSL \| 80-54 \| 2011 \| 2011BSRSL..80...54O \| http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80...54O 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis A. E. Chavushyan V. et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G 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 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 XMM-Newton serendipitous source catalogue \|Watson M. G. Pye J. P. et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W 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 A Detailed X-Ray Investigation of zeta Puppis. II. The Variability on Short and Long Timescales \|Naze Yael Oskinova Lidia M. \| ApJ \| 763-143 \| 2013 \| 2013ApJ...763..143N \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...763..143N Constraints on the Ubiquity of Coronal X-Ray Cycles \|Hoffman John Gunther Hans M. \| ApJ \| 759-145 \| 2012 \| 2012ApJ...759..145H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...759..145H A detailed X-ray investigation of zeta Puppis. III. Spectral analysis of the whole RGS spectrum \|Herve A. Rauw G. \| A&A \| 551-83 \| 2013 \| 2013A&A...551A..83H \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..83H Constraints on Porosity and Mass Loss in O-star Winds from the Modeling of X-Ray Emission Line Profile Shapes \|Leutenegger Maurice A. Cohen David H. et al. \| ApJ \| 770-80 \| 2013 \| 2013ApJ...770...80L \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...770...80L 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 Global Modeling of X-Ray Spectra Produced in O-type Star Winds \|Herve A. Rauw G. et al. \| ApJ \| 748-89 \| 2012 \| 2012ApJ...748...89H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748...89H 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 Interaction of the Fermi Bubbles with the Milky Ways 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 Perspectives for observing hot massive stars with XMM-Newton in the years 2017-2027 \|Rauw G. \| AN \| 338-207 \| 2017 \| 2017AN....338..207R \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..207R 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 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 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 An Observational Link between AGN Eddington Ratio and N IIu03bb6583/Hu03b1 at 0.6 < z < 1.7 \|Oh Kyuseok Ueda Yoshihiro et al. \| ApJ \| 880-112 \| 2019 \| 2019ApJ...880..112O \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...880..112O 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 Fe XVII 2p-3s Line Ratio Diagnostic of Shock Formation Radius in O Stars \|Grell Gabriel J. Leutenegger Maurice A. \| ApJ \| 917-105 \| 2021 \| 2021ApJ...917..105G \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...917..105G 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-06-08T01:33:58Z/2000-10-15T12:22:37Z
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	2001-12-29T00:00:00Z
Last Update	2025-01-27
Keywords	"resolution xray spectroscopy", "zeta puppis", "zeta pup", "hot stars", "bulk motion", "atmospheric densities", "total flux", "resolve velocity fields", "lin widths", "stellar surface", "rotationally modulated variations", "prototypical star", "wind structure", "pv program"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2001, 'High Resolution X-ray Spectroscopy of Zeta Puppis', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qotn320