The white dwarf cooling sequence in NGC 6791

Details The white dwarf cooling sequence in NGC 6791 The white dwarf cooling sequence in NGC 6791

2005-03-17

arxiv.org/abs/astro-ph/0503397v1

Astrophys.J. 624 (2005) L45-L48

Astronomy and Astrophysics

Astrophysics

11 pages, 3 figures. Accepted (2005 March 17) on ApJ Letter

Scientific paper

10.1086/430310

In the old, populous, and metal-rich open cluster NGC 6791 we have used deep HST/ACS images to track the white dwarf cooling sequence down to m_F606W~28.5. The white dwarf luminosity function shows a well defined peak at m_F606W~27.4, and a bending to the blue in the color--magnitude diagram. If this peak corresponds to the end of the white dwarf cooling sequence the comparison with theoretical isochrones provides a cluster age estimate of ~2.4 Gyr, in sharp contrast with the age of 8--9 Gyr inferred from the main-sequence turn-off. If the end is at fainter magnitudes, the peak at m_F606W~27.4 is even more enigmatic. We discuss possible causes, none of them very convincing.

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