A dataset provided by the European Space Agency

Name: GT Observations of Hot Stars: Iota Ori
Published: 2003-07-16T00:00:00Z

Proposal ID	011266
Title	GT Observations of Hot Stars: Iota Ori
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112660101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112660201
DOI	https://doi.org/10.5270/esa-y4dx7pf
Principal Investigator, PI	Dr Albert Brinkman
Abstract	GT-Iota Orion is a massive O-B binary in a highly eccentric orbit. Instabilitesin the individual winds and the collisions between the two winds are expectedto produce x-ray emitting shocked regions. With the high-resolution of the RGSwe will study the composition and structure of the two stellar winds as well asthe dynamics and emission mechanism of the collision regions. We willmap the complete field with the EPIC cameras to investigate X-ray emissionfrom young and forming stars.
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 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 Discovery of X-ray emission from the eclipsing brown-dwarf binary 2MASS J05352184-0546085 \|Czesla S. Schneider P. C. \| A&A \| 491-851 \| 2008 \| 2008A&A...491..851C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...491..851C 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 Million-Degree Plasma Pervading the Extended Orion Nebula \|Gudel Manuel Briggs Kevin R. et al. \| Sci \| 319-309 \| 2008 \| 2008Sci...319..309G \| http://ui.adsabs.harvard.edu/#abs/2008Sci...319..309G 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 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 Orion revisited. I. The massive cluster in front of the Orion nebula cluster \|Alves J. Bouy H. \| A&A \| 547-97 \| 2012 \| 2012A&A...547A..97A \| http://ui.adsabs.harvard.edu/#abs/2012A&A...547A..97A 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 An X-Ray Survey of the Young Stellar Population of the Lynds 1641 and Iota Orionis Regions \|Pillitteri I. Wolk S. J. et al. \| ApJ \| 768-99 \| 2013 \| 2013ApJ...768...99P \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...768...99P Young Stellar Objects in Lynds 1641: Disks Accretion and Star Formation History \|Fang Min Kim Jinyoung Serena et al. \| ApJS \| 207-5 \| 2013 \| 2013ApJS..207....5F \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..207....5F Transitional Disks and Their Origins: An Infrared Spectroscopic Survey of Orion A \|Kim K. H. Watson Dan M. et al. \| ApJ \| 769-149 \| 2013 \| 2013ApJ...769..149K \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...769..149K A New Halpha Emission-line Survey in the Orion Nebula Cluster \|Szegedi-Elek E. Kun M. et al. \| ApJS \| 208-28 \| 2013 \| 2013ApJS..208...28S \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...28S 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 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 NGC 1980 Is Not a Foreground Population of Orion: Spectroscopic Survey of Young Stars with Low Extinction in Orion A \|Fang Min Kim Jinyoung Serena et al. \| AJ \| 153-188 \| 2017 \| 2017AJ....153..188F \| http://ui.adsabs.harvard.edu/#abs/2017AJ....153..188F 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 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 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 EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2001-09-14T23:39:55Z/2001-09-15T08:15:28Z
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	2003-07-16T00:00:00Z
Last Update	2025-01-27
Keywords	"iota ori", "hot stars", "EPIC", "eccentric orbit", "individual winds", "forming stars", "emission mechanism", "xray emission", "iota orion", "complete field", "stellar winds", "epic cameras", "collision region"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2003, 'GT Observations of Hot Stars: Iota Ori', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y4dx7pf