2003ApJ...587L..31V


Query : 2003ApJ...587L..31V

2003ApJ...587L..31V - Astrophys. J., 587, L31-L34 (2003/April-2)

The slow temperature equilibration behind the shock front of SN 1006.

VINK J., LAMING J.M., GU M.F., RASMUSSEN A. and KAASTRA J.S.

Abstract (from CDS):

We report on the observation of O VII Doppler line broadening in a compact knot at the edge of SN 1006 detected with the reflective grating spectrometer on board XMM-Newton. The observed line width of σ=3.4±0.5 eV at a line energy of 574 eV indicates an oxygen temperature of kT=528±150 keV. Combined with the observed electron temperature of ∼1.5 keV, the observed broadening is direct evidence for temperature nonequilibration in high Mach number shocks and slow subsequent equilibration. The O VII line emission allows an accurate determination of the ionization state of the plasma, which is characterized by a relatively high forbidden line contribution, indicating logn_e_t≃9.2.

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Journal keyword(s): Shock Waves - ISM: Supernova Remnants - X-Rays: Individual: Alphanumeric: SN 1006

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 1572A SN* 00 25 21.5 +64 08 27           B8 1254 1
2 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
3 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1

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