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An Integral View of Balmer-dominated Shocks in Supernova Remnants

Published online by Cambridge University Press:  29 January 2014

Sladjana Nikolić ,
Glenn van de Ven ,
Kevin Heng ,
Daniel Kupko ,
Jose Alfonso Lopez Aguerri ,
Jairo Méndez-Abreu ,
Joan Font Serra  and
John Beckman
Sladjana Nikolić
Affiliation:
Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany email: [email protected]
Glenn van de Ven
Affiliation:
Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany email: [email protected]
Kevin Heng
Affiliation:
University of Bern, Center for Space and Habitability, Sidlerstrasse 5, Bern, Switzerland
Daniel Kupko
Affiliation:
Leibniz Institute for Astrophysics Potsdam (AIP), An der Sternwarte 16, Potsdam, Germany
Jose Alfonso Lopez Aguerri
Affiliation:
Instituto de Astrofísica de Canarias (IAC), Vía Láctea, La Laguna (Tenerife), Spain
Jairo Méndez-Abreu
Affiliation:
Instituto de Astrofísica de Canarias (IAC), Vía Láctea, La Laguna (Tenerife), Spain
Joan Font Serra
Affiliation:
Instituto de Astrofísica de Canarias (IAC), Vía Láctea, La Laguna (Tenerife), Spain
John Beckman
Affiliation:
Instituto de Astrofísica de Canarias (IAC), Vía Láctea, La Laguna (Tenerife), Spain
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Abstract

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We present integral-field spectroscopic observations with the VIMOS-IFU at the VLT of fast (2000-3000 kms−1) Balmer-dominated shocks surrounding the northwestern rim of the remnant of supernova 1006. The high spatial and spectral resolution of the instrument enable us to show that the physical characteristics of the shocks exhibit a strong spatial variation over few atomic scale lengths across 133 sky locations. Our results point to the presence of a population of non-thermal protons (10-100 keV) which might well be the seed particles for generating high-energy cosmic rays. We also present observations of Tycho's supernova remnant taken with the narrow-band tunable filter imager OSIRIS at the GTC and the Fabry-Perot interferometer GHaFaS at the WHT to resolve respectively the broad and narrow Hα lines across a large part of the remnant.

Keywords

Balmer emissionsupernova remnantscosmic raysintegral-field spectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 165 - 169
Copyright
Copyright © International Astronomical Union 2014 

References

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