On the abundance of Lithium in T Coronae Borealis

Astronomy and Astrophysics – Astrophysics

Scientific paper

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3 pages, 1 figure (a and b), accepted by MNRAS

Scientific paper

10.1046/j.1365-8711.1999.02549.x

We have obtained high resolution echelle spectroscopy of the recurrent nova T CrB. We find that the surface lithium abundance in T CrB is signifcantly enhanced compared to field M giants, where it is not detectable. We offer possible explanations for this in terms of either a delay in the onset of convection in the giant star, enhanced coronal activity due to star-spots or the enhancement of Li resulting from the nova explosion(s).

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