Maurizio Salaris

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Leandro G Althaus1
René D Rohrmann1
1Leandro G Althaus
1René D Rohrmann
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NGC 6791 is a well studied open cluster that it is so close to us that can be imaged down to very faint luminosities. The main-sequence turn-off age ( approximately 8 Gyr) and the age derived from the termination of the white dwarf cooling sequence ( approximately 6 Gyr) are very different. One possible explanation is that as white dwarfs cool, one of the(More)
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