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Two Extrasolar Asteroids with Low Volatile-element Mass Fractions

  • Authors: M. Jura, S. Xu(许偲艺), B. Klein, D. Koester, and B. Zuckerman

Jura et al. 2012 The Astrophysical Journal 750 69.

  • Provider: AAS Journals

Caption: Figure 2.

Similar to Figure 1, except for C i and C ii. For G241-6, the C ii line at 1334.53 Å is shifted by +19 km s −1 with respect to the photospheric velocity; likely it is largely interstellar. We regard the C i lines to be undetected in both stars.

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