High Resolution X-Ray Spectroscopy of SN 1987A: Monitoring with XMM-Newton

Abstract

We report the results of our XMM-Newton monitoring of SN 1987A. The ongoing propagation of the supernova blast wave through the inner circumstellar ring caused a drastic increase in X-ray luminosity during the last years, enabling detailed high resolution X-ray spectroscopy with the Reflection Grating Spectrometer. The observations can be used to follow the detailed evolution of the arising supernova remnant. The fluxes and broadening of the numerous emission lines seen in the dispersed spectra provide information on the evolution of the X-ray emitting plasma and its dynamics. These were analyzed in combination with the EPIC-pn spectra, which allow a precise determination of the higher temperature plasma. We modeled individual emission lines and fitted plasma emission models. Especially from the observations between 2003 and 2007 we can see a significant evolution of the plasma parameters and a deceleration of the radial velocity of the lower temperature plasma regions. We found an indication (3-sigma-level) of an iron K feature in the co-added EPIC-pn spectra. The comparison with Chandra grating observations in 2004 yields a clear temporal coherence of the spectral evolution and the sudden deceleration of the expansion velocity seen in X-ray images ~6100 days after the explosion.

10 pages, 8 Figures; accepted by A&A

References in corpus (22)

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• Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots
• X-ray Evolution of SNR 1987A: The Radial Expansion
• Chandra LETG Observations of Supernova Remnant 1987A
• Fourier Modeling of the Radio Torus Surrounding Supernova 1987A
• XMM-Newton observations of SN1987A
• Chandra HETG Spectra of SN 1987A at 20 years
• Chandra Observations of Shock Kinematics in Supernova Remnant 1987A
• Evolution of the Reverse Shock Emission from SNR 1987A
• Probing Elemental Abundances in SNR 1987A Using XMM-Newton
• Coronal emission from the shocked circumstellar ring of SN 1987A
• Fifteen Years of High-Resolution Radio Imaging of Supernova 1987A
• X-ray Evolution of SN 1987A

Cited by in corpus (19)

• The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
• Herschel Detects a Massive Dust Reservoir in Supernova 1987A
• A stubbornly large mass of cold dust in the ejecta of Supernova 1987A
• The timing and location of dust formation in the remnant of SN 1987A
• The population of X-ray supernova remnants in the Large Magellanic Cloud
• Hard X-ray emission lines from the decay of Ti-44 in the remnant of supernova 1987A
• XMM-Newton study of 30 Dor C and a newly identified MCSNR J0536-6913 in the Large Magellanic Cloud
• XMM-Newton observations of SNR 1987A. II. The still increasing X-ray light curve and the properties of Fe K lines
• Thermal Emission and Radioactive Lines, but No Pulsar, in the Broadband X-Ray Spectrum of Supernova 1987A
• A New Evolutionary Phase of Supernova Remnant 1987A
• Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-Resolution $Chandra$ HETG Study
• The Post-impact Evolution of the X-ray Emitting Gas in SNR 1987A Viewed by XMM-Newton
• SN 1987A : Tracing the flux decline and spectral evolution through a comparison of SRG/eROSITA and XMM-Newton observations
• Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring
• The Exceptional X-ray Evolution of SN1996cr in High Resolution
• X-ray Decay Lines from Heavy Nuclei in Supernova Remnants as a Probe of the r-Process Origin and the Birth Periods of Magnetars
• The Luminosity Phase Space of Galactic and Extragalactic X-ray Transients Out to Intermediate Redshifts
• Kinematics of Supernova Remnants: Status of X-Ray Observations
• Unusual X-ray Oxygen Line Ratios of SN 1987A Arising From the Absorption of Galactic Hot Interstellar Medium