2000ApJS..127..233B


Query : 2000ApJS..127..233B

2000ApJS..127..233B - Astrophys. J., Suppl. Ser., 127, 233-237 (2000/April-0)

X-ray emission from comets, cometary knots, and supernova remnants.

BINGHAM R., KELLETT B.J., DAWSON J.M., SHAPIRO V.D. and MENDIS D.A.

Abstract (from CDS):

A comparison is made between one of the processes leading to cometary X-ray emission and X-rays from supernova remnants. We demonstrate that the X-ray emission in both comet and supernova is bremsstrahlung and line radiation created by energetic electrons accelerated by plasma turbulence. We further demonstrate that the most likely source of plasma turbulence is produced by counterstreaming ion populations which result from the mass loading effect or from an anisotropic distribution produced by reflecting ions from a collisionless shock. The instability that gives rise to the plasma turbulence is the modified two-stream instability of counterstreaming ions. A similar instability arises in laser-plasma interactions that have self-generating magnetic fields and flowing ions.

Abstract Copyright: ∼

Journal keyword(s): Comets: General - Instabilities - Radiation Mechanisms: Nonthermal - ISM: Supernova Remnants - Turbulence - X-Rays: General

Simbad objects: 2

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Number of rows : 2
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 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
2 NGC 7293 PN 22 29 38.5454047152 -20 50 13.747242408 11.894 13.158 13.524 13.689 13.898 DAO.5 983 1

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