Chandra HETG Spectra of SN 1987A at 20 years
arXiv:0802.2340 · doi:10.1086/587549
Abstract
We have undertaken deep, high-resolution observations of SN 1987A at ~20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise in the 6 A to 20 A bandpass, which includes the H-like and He-like lines of Si, Mg, Ne, as well as O VIII lines and bright Fe XVII lines. In joint analysis with LETG data, we find that there has been a significant decrease from 2004 to 2007 in the average temperature of the highest temperature component of the shocked-plasma emission. Model fitting of the profiles of individual HETG lines yields bulk kinematic velocities of the higher-Z ions, Mg and Si, that are significantly lower than those inferred from the LETG 2004 observations.
arXiv comment12 pages, 5 figures, 1 table; accepted for publication in ApJ Letters
References in corpus (9)
- The X-ray Spectrum of Supernova Remnant 1987A
- Evolutionary Status of SNR 1987A at the Age of Eighteen
- Chandra LETG Observations of Supernova Remnant 1987A
- XMM-Newton observations of SN1987A
- Chandra Observations of Shock Kinematics in Supernova Remnant 1987A
- X-ray Spectroscopy of the Contact Binary VW Cephei
- Chandra Observations of Supernova 1987A
- Dust-Gas Interaction in SNR 1987A
- X-ray Evolution of SN 1987A
Cited by in corpus (22)
- Supernova remnants: the X-ray perspective
- Thermal and non-thermal emission from circumstellar interaction
- Abundances and density structure of the inner circumstellar ring around SN 1987A
- Collisionless shock heating of heavy ions in SN 1987A
- High-Resolution X-ray Spectroscopy of SNR 1987A: Chandra LETG and HETG Observations in 2007
- 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
- Wavelength Measurements of K Transitions of Oxygen, Neon, and Magnesium with X-ray Absorption Lines
- Evolution of the Chandra CCD Spectra of SNR 1987A: Probing the Reflected-Shock Picture
- High Resolution X-Ray Spectroscopy of SN 1987A: Monitoring with XMM-Newton
- 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
- The Morphologies and Kinematics of Supernova Remnants
- A New Evolutionary Phase of Supernova Remnant 1987A
- Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-Resolution HETG Study
- X-ray ejecta kinematics of the Galactic core-collapse supernova remnant G292.0+1.8
- X-Ray and Gamma-Ray Emission From Core-collapse Supernovae: Comparison of Three-dimensional Neutrino-driven Explosions With SN 1987A
- High-cadence Dispersed Spectral Analysis of Supernova Remnant 1987A
- Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring
- The Exceptional X-ray Evolution of SN1996cr in High Resolution
- Kinematics of Supernova Remnants: Status of X-Ray Observations
- Massive stars as thermonuclear reactors and their explosions following core collapse