High resolution X-ray spectroscopy of SN1987 A: monitoring with XMM-Newton

作者：Sturm R^*; Haberl F; Aschenbach B; Hasinger G

来源：Astronomy & Astrophysics, 2010, 515: A5.

DOI：10.1051/0004-6361/200913317

• ISM: supernova remnants
• supernovae: general
• supernovae: individual: SN1987 A
• X-rays: general
• X-rays: stars
• shock waves

Context. The ongoing propagation of the supernova blast wave of SN1987 A through its inner circumstellar ring has caused a drastic increase in X-ray luminosity in the past few years, which has allowed detailed high resolution X-ray spectroscopy to be performed with the Reflection Grating Spectrometer.
Aims. We report the results of our XMM-Newton monitoring of SN1987A, which may be used to follow the detailed evolution of the arising supernova remnant.
Methods. The fluxes and broadening of the numerous emission lines measured in the dispersed spectra provide information about 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.
Results. For observations between 2003 and 2007 in particular, we detect significant evolution in the plasma parameters and a deceleration of the radial velocity in the lower temperature plasma regions. We detected (at 3 sigma-level) an iron K feature in the coadded EPIC-pn spectra.
Conclusions. By comparing with Chandra grating observations in 2004, we observe a clear temporal coherence of the spectral evolution and the sudden deceleration of the expansion velocity detectable in X-ray images similar to 6100 days after the explosion.

• 出版日期2010-6