{ "id": "astro-ph/0210572", "version": "v1", "published": "2002-10-25T17:04:46.000Z", "updated": "2002-10-25T17:04:46.000Z", "title": "Far Ultraviolet Spectra of a Non-Radiative Shock Wave in the Cygnus Loop", "authors": [ "John Raymond", "Parviz Ghavamian", "Ravi Sankrit", "William Blair", "Salvador Curiel" ], "comment": "To appear in Astrophysical Journal, Vol. 584, Feb. 20 2003", "journal": "Astrophys.J. 584 (2003) 770-781", "doi": "10.1086/345741", "categories": [ "astro-ph" ], "abstract": "Spatial and spectral profiles of O VI emission behind a shock wave on the northern edge of the Cygnus Loop were obtained with the FUSE satellite. The velocity width of the narrowest O VI profile places a tight constraint on the electron-ion and ion-ion thermal equilibration in this 350 $\\rm km s^{-1}$ collisionless shock. Unlike faster shocks in SN1006 and in the heliosphere, this shock brings oxygen ions and protons to within a factor of 2.5 of the same temperature. Comparison with other shocks suggests that shock speed, rather than Alfv\\'{e}n Mach number, may control the degree of thermal equilibration. We combine the O VI observations with a low resolution far UV spectrum from HUT, an H$\\alpha$ image and ROSAT PSPC X-ray data to constrain the pre-shock density and the structure along the line-of-sight. As part of this effort, we model the effects of resonance scattering of O VI photons within the shocked gas and compute time-dependent ionization models of the X-ray emissivity. Resonance scattering affects the O VI intensities at the factor of 2 level, and the soft spectrum of the X-ray rim can be mostly attributed to departures from ionization equilibrium. The pre-shock density is about twice the canonical value for the Cygnus Loop X-ray emitting shocks.", "revisions": [ { "version": "v1", "updated": "2002-10-25T17:04:46.000Z" } ], "analyses": { "keywords": [ "cygnus loop", "far ultraviolet spectra", "non-radiative shock wave", "loop x-ray emitting shocks", "low resolution far uv spectrum" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 600602 } } }