A dataset provided by the European Space Agency

Name: The fragments of the Vela SNR progenitor and RX J0882.0-4622
Published: 2002-09-03T00:00:00Z

Proposal ID	011287
Title	The fragments of the Vela SNR progenitor and RX J0882.0-4622
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112870801
DOI	https://doi.org/10.5270/esa-oagqbl2
Principal Investigator, PI	Dr Bernd Aschenbach
Abstract	GT- In the ROSAT all-sky survey X-ray emitting protrusions outside the boundary of the Vela SNR have been discovered. They appear to be fragments of theprogenitor star and they should be enriched in heay elements, which has beenconfirmed by ASCA observations but limited by statistics. With XMM we will takespatially resolved spectra of the fragments to clarify the elemental enhancementand the spatial distribution resulting from the mixing with ISM matter. In thesoutheastern part of the Vela SNR a new young SNR at a short distance has beendiscovered with ROSAT and GRO, which emits 44-Ti; according to ASCA observationsthe source appears to emit just spectra of the power-law type. It is essentialto search for emission lines and determine the precise shape of the continuum.
Publications	XMM-Newton observations of the supernova remnant RX J0852.0-4622/GRO J0852-4642 \|Iyudin, A. F., Aschenbach, B., et al. \| A&A \| 429-225 \| 2005 \| 2005A&A...429..225I \| http://ui.adsabs.harvard.edu/#abs/2005A&A...429..225I 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 Is Vela Jr. a young supernova remnant? \|Katsuda, Satoru, Tsunemi, Hiroshi, \| AdSpR \| 43-895 \| 2009 \| 2009AdSpR..43..895K \| http://ui.adsabs.harvard.edu/#abs/2009AdSpR..43..895K Identifying XMM-Newton observations affected by solar wind charge exchange. Part I \|Carter, J. A., Sembay, S., \| A&A \| 489-837 \| 2008 \| 2008A&A...489..837C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...489..837C Spatially Resolved X-Ray Spectroscopy of Vela Shrapnel A \|Katsuda, S., Tsunemi, H., \| ApJ \| 642-917 \| 2006 \| 2006ApJ...642..917K \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...642..917K 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 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 Origin of the shrapnels around the Vela SNR \|Tsunemi, Hiroshi, Katsuda, Satoru, \| NewAR \| 50-521 \| 2006 \| 2006NewAR..50..521T \| http://ui.adsabs.harvard.edu/#abs/2006NewAR..50..521T 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 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 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 new nearby pulsar wind nebula overlapping the RX J0852.0-4622 supernova remnant \|Acero, F., Gallant, Y., et al. \| A&A \| 551-7 \| 2013 \| 2013A&A...551A...7A \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A...7A Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622 \|Kishishita, T., Hiraga, J., \| A&A \| 551-132 \| 2013 \| 2013A&A...551A.132K \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A.132K 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-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 A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars \|Pye, J. P., Rosen, S., et al. \| A&A \| 581-28 \| 2015 \| 2015A&A...581A..28P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...581A..28P 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 The Slow X-Ray Expansion of the Northwestern Rim of the Supernova Remnant RX J0852.0-4622 \|Katsuda, S., Tsunemi, H., \| ApJ \| 678-35 \| 2008 \| 2008ApJ...678L..35K \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...678L..35K 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 Systematic Study of Acceleration Efficiency in Young Supernova Remnants with Nonthermal X-Ray Observations \|Tsuji, Naomi, Uchiyama, Yasunobu, et al. \| ApJ \| 907-117 \| 2021 \| 2021ApJ...907..117T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907..117T 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 SRG/eROSITA and XMM-Newton observations of Vela Jr \|Camilloni, Francesco, Becker, Werner, et al. \| A&A \| 673-45 \| 2023 \| 2023A&A...673A..45C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..45C A Statistical Study of Soft X-Ray Flares on Solar-type Stars \|Zhao, Z. H., Hua, Z. Q., et al. \| ApJ \| 961-130 \| 2024 \| 2024ApJ...961..130Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..130Z 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	2000-12-07T14:41:18Z/2001-04-27T19:27:45Z
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	2002-09-03T00:00:00Z
Keywords	"source appears", "short distance", "supernova remnant", "XMM", "progenitor star", "heay elements", "emission lines", "vela supernova remnant", "precise shape", "J0882.0", "spatial distribution", "ism matter", "rx j0882", "resolved spectra", "elemental enhancement", "power law type", "ROSAT"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bernd Aschenbach, 2002, 'The fragments of the Vela SNR progenitor and RX J0882.0-4622', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-oagqbl2