A dataset provided by the European Space Agency

Name: Hot Gas in Wind Blown Bubbles
Published: 2002-12-31T00:00:00Z

Proposal ID	007957
Title	Hot Gas in Wind Blown Bubbles
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0079570201
DOI	https://doi.org/10.5270/esa-zf7by7s
Principal Investigator, PI	Prof You-Hua Chu
Abstract	Fast stellar winds from massive stars sweep up the surrounding gas to form bubbles. The shocked stellar wind reaches X-ray-emitting temperatures. Onlytwo wind-blown bubbles have been confirmed to emit diffuse X-rays: NGC 6888and S 308. Both bubbles are blown by Wolf-Rayet stars, and both contain processed stellar material ejected by their progenitors. The observed X-rayfluxes of both NGC 6888 and S308 are lower than model predictions by orders ofmagnitude. The high spatial and spectral resolutions of the XMM instrumentsprovide an opportunity to monumentally improve the quality of the X-ray observations so that a comprehensive investigation of a bubble is possible.We request XMM observations of S 308 in this AO and NGC 6888 in the future.
Publications	On the nature of Collinder 121: insights from the low-mass pre-main sequence \|Burningham, Ben, Naylor, Tim, et al. \| MNRAS \| 346-1143 \| 2003 \| 2003MNRAS.346.1143B \| http://ui.adsabs.harvard.edu/#abs/2003MNRAS.346.1143B 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 The XMM-Newton EPIC background: Production of background maps and event files \|Read, A. M., Ponman, T. J., \| A&A \| 409-395 \| 2003 \| 2003A&A...409..395R \| http://ui.adsabs.harvard.edu/#abs/2003A&A...409..395R XMM-Newton data processing for faint diffuse emission. Proton flares, exposure maps and report on EPIC MOS1 bright CCDs contamination \|Pradas, J., Kerp, J., \| A&A \| 443-721 \| 2005 \| 2005A&A...443..721P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...443..721P The XMM-Newton EPIC background and the production of background blank sky event files \|Carter, J. A., Read, A. M., \| A&A \| 464-1155 \| 2007 \| 2007A&A...464.1155C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...464.1155C Hot Gas in the Circumstellar Bubble S308 \|Chu, You-Hua, Guerrero, Martin A., et al. \| ApJ \| 599-1189 \| 2003 \| 2003ApJ...599.1189C \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...599.1189C 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 Constraints on sterile neutrinos as dark matter candidates from the diffuse X-ray background \|Boyarsky, A., Neronov, A., et al. \| MNRAS \| 370-213 \| 2006 \| 2006MNRAS.370..213B \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.370..213B 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 X-Ray Emission from the Wolf-Rayet Bubble S 308 \|Toala, J. A., Guerrero, M. A., et al. \| ApJ \| 755-77 \| 2012 \| 2012ApJ...755...77T \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...755...77T 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 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 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 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 Decaying fermionic warm dark matter and XENON1T electronic recoil excess \|Dutta, Koushik, Ghosh, Avirup, et al. \| PDU \| 33-100855 \| 2021 \| 2021PDU....3300855D \| http://ui.adsabs.harvard.edu/#abs/2021PDU....3300855D 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2001-10-23T22:01:22Z/2001-10-24T12:36:18Z
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	2002-12-31T00:00:00Z
Keywords	"xray emitting temperatures", "wolf rayet stars", "hot gas", "NGC 6888", "XMM", "massive stars sweep", "spectral resolutions", "comprehensive investigation", "fast stellar winds", "xmm instruments", "emit diffuse xray", "wind blown bubbles", "ngc 6888", "form bubbles", "shocked stellar wind", "xray fluxes", "model predictions", "processed stellar material"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof You-Hua Chu, 2002, 'Hot Gas in Wind Blown Bubbles', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zf7by7s