High resolution spectroscopy of Balmer-dominated shocks in the RCW 86, Kepler and SN 1006 supernova remnants

We report results from high resolution optical spectroscopy of three non-radiative galactic supernova remnants, RCW 86, Kepler's supernova remnant and SN 1006. We have measured the narrow component Hα line widths in Balmer-dominated filaments in RCW 86 and SN 1006, as well as the narrow component width in a Balmer-dominated knot in Kepler's SNR. The narrow component line widths measured in RCW 86 and Kepler's SNR show FWHM of 30-40 km s-1, similar to what has been seen in other Balmer-dominated remnants. Of the remnants in our sample, SN 1006 is the fastest shock ( ~ 3000 km s-1). The narrow component Hα and Hβ lines in this remnant have a FWHM of merely 21 km s-1. Comparing the narrow component widths measured in our sample with those measured in other remnants shows that the width of the narrow component does not correlate in a simple way with the shock velocity. The implications for the pre-heating mechanism responsible for the observed line widths are discussed. Based on observations collected at the European Southern Observatory, Paranal, Chile (ESO Programme 67.D-0579).

Ghavamian, P. (författare)
Lundqvist, P.Stockholms universitet,Institutionen för astronomi(Swepub:su)lundq (författare)
Smith, R. C. (författare)
Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Ingår i:Astronomy and Astrophysics: EDP Sciences407, s. 249-2570004-63611432-0746

Av författaren/redakt...: Sollerman, J.; Ghavamian, P.; Lundqvist, P.; Smith, R. C.

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