The outer wind of gamma Velorum
Fine-structure mid-infrared emission lines with critical densities in the regime 10 4 ≤ n crit ≤ 10 6cm -3 can be employed to probe the outflow from Wolf-Rayet (WR) stars at radii of ~10 15cm. Narrow-band mid-infrared imaging and spectroscopy of the nearest WR star to the Sun, γVelorum is analysed f...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2012
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