FUSE Observations of High-Velocity Gas Toward the Vela SNR

Details FUSE Observations of High-Velocity Gas Toward the Vela SNR FUSE Observations of High-Velocity Gas Toward the Vela SNR

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.8211n&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #82.11; Bulletin of the American Astronomical Society, Vol. 32, p.1541

Astronomy and Astrophysics

Astronomy

Scientific paper

FUSE far-UV spectra toward 7 stars in the line of sight to the Vela supernova remnant reveal high-velocity components to the interstellar line of O VI. These high velocity components are in general consistent with high velocity features seen in C IV toward these same target stars with IUE. We correlate the velocities and column densities of the O VI features with those of C IV and discuss the implications for the shock velocity and interstellar environment of the Vela supernova remnant.

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