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., Vel\\u00e1zquez, 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
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
Keywords	"archival asca data", "supernova remnant", "XMM", "ejecta abundance", "ionized ne", "ne ejecta", "perform spectroscopic", "west limb", "XMM-Newton", "ne rich ejecta", "angular resolution", "interstellar medium", "xray emitting ejecta", "neon rich ejecta", "xmm newton"
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