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A consistency test of white dwarf and main sequence ages: NGC 6791.
- Source :
- EPJ Web of Conferences; 2013, Issue 43, p05003-p.1-05003-p.3, 3p
- Publication Year :
- 2013
-
Abstract
- NGC 6791 is an open cluster that it is so close to us that can be imaged down to very faint luminosities. The main sequence turn-off age (~8 Gyr) and the age derived from the cut-off of the white dwarf luminosity function (~6 Gyr) were found to be significantly different. Here we demonstrate that the origin of this age discrepancy lies in an incorrect evaluation of the white dwarf cooling ages, and we show that when the relevant physical separation processes are included in the calculation of white dwarf sequences both ages are coincident. [ABSTRACT FROM AUTHOR]
- Subjects :
- WHITE dwarf stars
STAR clusters
STELLAR luminosity function
GALAXIES
ASTRONOMY
Subjects
Details
- Language :
- English
- ISSN :
- 21016275
- Issue :
- 43
- Database :
- Complementary Index
- Journal :
- EPJ Web of Conferences
- Publication Type :
- Conference
- Accession number :
- 86427031
- Full Text :
- https://doi.org/10.1051/epjconf/20134305003