A dataset provided by the European Space Agency

Name: Neon-rich Ejecta in the West Limb of the Puppis A Supernova Remnant
Published: 2006-11-11T00:00:00Z

Proposal ID	030353
Title	Neon-rich Ejecta in the West Limb of the Puppis A Supernova Remnant
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303530101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303530201
DOI	https://doi.org/10.5270/esa-edt6u2t
Principal Investigator, PI	Prof Koji Mori
Abstract	We propose a 30 ksec observation of the west limb of the Puppis A supernovaremnant to study Ne-rich ejecta. We discovered evidence of enhanced X-ray lineemission from highly ionized Ne in archival ASCA data, but otherwise, Puppis Adoes not yield direct evidence of X-ray emitting ejecta. The good angularresolution and high throughput of XMM-Newton will enable us to isolate the Neejecta from the surrounding interstellar medium and perform spectroscopicstudies to measure the ejecta abundances. This program thus provides a uniqueopportunity to study the X-ray emitting nucleosynthesis products in Puppis A.
Publications	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 Discovery of X-ray-emitting O-Ne-Mg-rich Ejecta in the Galactic Supernova Remnant Puppis A \|Katsuda Satoru Hwang Una et al. \| ApJ \| 714-1725 \| 2010 \| 2010ApJ...714.1725K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714.1725K The most complete and detailed X-ray view of the SNR Puppis A \|Dubner G. Loiseau N. et al. \| A&A \| 555-9 \| 2013 \| 2013A&A...555A...9D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A...9D 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 Feature-tailored spectroscopic analysis of the supernova remnant Puppis A in X-rays \|Luna G. J. M. Smith M. J. S. et al. \| A&A \| 590-70 \| 2016 \| 2016A&A...590A..70L \| http://ui.adsabs.harvard.edu/#abs/2016A&A...590A..70L Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions \|Katsuda Satoru Morii Mikio et al. \| ApJ \| 856-18 \| 2018 \| 2018ApJ...856...18K \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...856...18K Wide-field X-ray observations of the supernova remnant Puppis A with the SRG/ART-XC telescope \|Krivonos R. Arefiev V. et al. \| MNRAS \| 510-3113 \| 2022 \| 2022MNRAS.510.3113K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.510.3113K Rectangular core-collapse supernova remnants: application to Puppis A \|Meyer D. M. -A. Velu00e1zquez P. F. et al. \| MNRAS \| 515-594 \| 2022 \| 2022MNRAS.515..594M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515..594M The Peculiar Ejecta Rings in the O-Rich Supernova Remnant Puppis A: Evidence of a Binary Interaction? \|Ghavamian Parviz Seitenzahl Ivo R. et al. \| ApJ \| 960-7 \| 2024 \| 2024ApJ...960....7G \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...960....7G Progenitors and Explosion Properties of Supernova Remnants Hosting Central Compact Objects \|Braun Chelsea \| PhDT \| 0-5 \| 2023 \| 2023PhDT.........5B \| http://ui.adsabs.harvard.edu/#abs/2023PhDT.........5B
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2005-10-09T02:29:20Z/2005-10-09T15:00:08Z
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	2006-11-11T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "XMM-Newton", "ejecta abundance", "perform spectroscopic", "neon rich ejecta", "xmm newton", "interstellar medium", "west limb", "angular resolution", "xray emitting ejecta", "ne rich ejecta", "archival asca data", "ne ejecta", "ionized ne", "supernova remnant"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Koji Mori, 2006, 'Neon-rich Ejecta in the West Limb of the Puppis A Supernova Remnant', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-edt6u2t