Spectroscopy of the remnant of supernova 1006

Details Spectroscopy of the remnant of supernova 1006 Spectroscopy of the remnant of supernova 1006

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244..517l&link_type=abstract

Astrophysical Journal, Part 1, vol. 244, Mar. 1, 1981, p. 517-519.

Astronomy and Astrophysics

Astrophysics

17

Astronomical Spectroscopy, H Alpha Line, Nebulae, Shock Fronts, Supernova Remnants, Interstellar Matter

Scientific paper

New spectroscopic results establish the absence of a broad component to H alpha in the remnant on SN 1006. This result implies a collisionless shock faster than 2700 km/sec in the theory of Chevalier and Raymond (1978). A consistent interpretation of Tycho's remnant and SNR 1006, based upon the collisionless shock theory and density fluctuations in the interstellar medium, is offered.

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