A dataset provided by the European Space Agency

Name: The Nature of the Vela SNR X-ray Emission
Published: 2002-11-25T00:00:00Z

Proposal ID	011269
Title	The Nature of the Vela SNR X-ray Emission
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112690101
DOI	https://doi.org/10.5270/esa-xehacow
Principal Investigator, PI	Dr Martin Turner
Abstract	GT-We propose to observe two filaments in the shock region of the Vela SupernovaRemnant which we have already observed in the optical and in the X-Ray band(with ROSAT/PSPC). We have found out that there is a strong evidence of shock-ISM inhomogeneities interaction, but the low spatial and spectral resolution ofPSPC data prevented us to study the real nature of the X-ray emission. In particular, our primary goal is to carry on spatially resolved spectral analysison a 1x1 arcmin resolution element of the post-shock region. This will allow usto discriminate clearly between the interaction processes, either evaporative orbow shock or secondary shocks, to derive the metal abundances behind the shock,and to understand the connection between different ISM phases.
Publications	Shock-cloud interaction in the Vela SNR observed with XMM-Newton \|Miceli, M., Bocchino, F., et al. \| A&A \| 442-513 \| 2005 \| 2005A&A...442..513M \| http://ui.adsabs.harvard.edu/#abs/2005A&A...442..513M 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 Probing the Nature of the Vela X Cocoon \|LaMassa, Stephanie M., Slane, Patrick O., \| ApJ \| 689-121 \| 2008 \| 2008ApJ...689L.121L \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...689L.121L Shock-cloud interaction in the Vela SNR. II. Hydrodynamic model \|Miceli, M., Reale, F., et al. \| A&A \| 458-213 \| 2006 \| 2006A&A...458..213M \| http://ui.adsabs.harvard.edu/#abs/2006A&A...458..213M Physical and Chemical Inhomogeneities inside the Vela SNR Shell: Indications of Ejecta Shrapnels \|Miceli, M., Bocchino, F., \| ApJ \| 676-1064 \| 2008 \| 2008ApJ...676.1064M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...676.1064M 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 Shock-cloud interactions in the Vela SNR: preliminary results of an XMM-Newton observation \|Bocchino, F., Miceli, M., \| AdSpR \| 33-381 \| 2004 \| 2004AdSpR..33..381B \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..33..381B Multi-phase interstellar clouds in the Vela SNR resolved with XMM-Newton \|Miceli, M., Bocchino, F., et al. \| AdSpR \| 35-1012 \| 2005 \| 2005AdSpR..35.1012M \| http://ui.adsabs.harvard.edu/#abs/2005AdSpR..35.1012M 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 The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 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 Multiwavelength Observations of Pulsar Wind Nebulae \|Slane, Patrick, \| ASSP \| 21-373 \| 2011 \| 2011ASSP...21..373S \| http://ui.adsabs.harvard.edu/#abs/2011ASSP...21..373S High Resolution X-ray Observations of Supernova Remnants \|Bocchino, F., \| ChJAS \| 3-329 \| 2003 \| 2003ChJAS...3..329B \| http://ui.adsabs.harvard.edu/#abs/2003ChJAS...3..329B 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 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	2001-11-09T01:22:56Z/2001-11-09T10:11:07Z
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	2002-11-25T00:00:00Z
Keywords	"xray band", "interaction processes", "resolved spectral analysis", "metal abundance", "secondary shoc", "vela supernova remnant", "pspc data prevented", "bow shock", "low spatial", "post shock region", "shock region", "ism phases", "xray emission", "spectral resolution", "ROSAT"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Martin Turner, 2002, 'The Nature of the Vela SNR X-ray Emission', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xehacow