The sealing of fragmenting shells - evidence from optical studies of the VELA remnant

Details The sealing of fragmenting shells - evidence from optical studies of the VELA remnant The sealing of fragmenting shells - evidence from optical studies of the VELA remnant

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.230..243m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 230, Jan. 15, 1988, p. 243-247.

Astronomy and Astrophysics

Astronomy

13

Forbidden Transitions, H Alpha Line, Nitrogen Ions, Stellar Envelopes, Supernova Remnants, Density Distribution, Echelette Gratings, Thermal Stability, Velocity Distribution

Scientific paper

Echelle spectra of H-alpha and forbidden N II emission show that a
fragmenting shell in the Vela supernova remnant is sealed by a blister.
The existence of blisters on a remnant shell can produce an unexpected
relationship between the velocities of features detected in absorption
and position on the shell.

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