A dataset provided by the European Space Agency

Name: Imaging the outflow of 2 MK gas from the Orion Nebula
Published: 2010-09-12T00:00:00Z

Proposal ID	060590
Title	Imaging the outflow of 2 MK gas from the Orion Nebula
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605900101
DOI	https://doi.org/10.5270/esa-j5n4obl
Principal Investigator, PI	Dr Kevin Briggs
Abstract	Our discovery of diffuse X-ray emission in the Orion Nebula has demonstratedthat hot bubbles, created by shocks in the powerful, hypersonic winds of high-mass stars, are a common feature of high-mass star-forming regions, not onlythose that host many early O-type stars. Pressure equilibrium with the HII gasand an apparent stream of 1.8 MeV emission, caused by the radioactive decay of26Al, connecting the Nebula region to the nearby Eridanus Superbubble suggestthe hot gas is not confined. The outflow of hot gas from such regions couldprovide a continual source of enrichment of the ISM, complementary to thediscrete but rare input of supernovae. Our aim is to directly image the outflowof X-ray-emitting hot gas from the Orion Nebula.
Publications	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 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 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 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 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 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	2009-08-28T10:47:57Z/2009-08-29T13:29:39Z
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	2010-09-12T00:00:00Z
Last Update	2025-01-27
Keywords	"mev emission", "apparent stream", "continual source", "type stars", "diffuse xray emission", "pressure equilibrium", "orion nebula", "mk gas", "nebula region", "hot bubbles", "hypersonic winds", "hii gas", "nearby eridanus superbubble", "hot gas", "mass stars", "radioactive decay", "rare input"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kevin Briggs, 2010, 'Imaging the outflow of 2 MK gas from the Orion Nebula', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j5n4obl