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Paper detail

The post-nova population

We here present our on-going project to unveil the post-nova population by re-discovering old novae that have been lost after the initial outburst and of which the binary itself is unobserved. We take UBVR photometry for the candidate selection, long-slit spectroscopy to confirm these candidates, and time-resolved spectroscopy to measure the orbital period of the newly confirmed post-novae. Some preliminary results are shown as examples.

preprint2011arXivOpen access
Linda SchmidtobreickClaus TappertAlessandro EderocliteNikolaus Vogt
astro-ph.SR
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Linda SchmidtobreickClaus TappertAlessandro EderocliteNikolaus Vogt

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