The Initial-Final Mass Relationship: Spectroscopy of White Dwarfs in NGC 2099 (M37)

This publication has 20 references indexed in Scilit:

• The Dearth of Massive, Helium-rich White Dwarfs in Young Open Star Clusters
  The Astrophysical Journal, 2004
• The CFHT Open Star Cluster Survey. IV. Two Rich, Young Open Star Clusters: NGC 2168 (M35) and NGC 2323 (M50)
  The Astronomical Journal, 2003
• The Masses of White Dwarfs in the Praesepe Open Cluster
  The Astrophysical Journal, 2001
• The CFHT Open Star Cluster Survey. III. The White Dwarf Cooling Age of the Rich Open Star Cluster NGC 2099 (M37)
  The Astronomical Journal, 2001
• The CFHT Open Star Cluster Survey. II. Deep CCD Photometry of the Old Open Star Cluster NGC 6819
  The Astronomical Journal, 2001
• The Potential of White Dwarf Cosmochronology
  Publications of the Astronomical Society of the Pacific, 2001
• Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
  Monthly Notices of the Royal Astronomical Society, 2000
• Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 $M_{\odot}$, and from $Z=0.0004$ to 0.03
  Astronomy and Astrophysics Supplement Series, 2000
• On the initial-final mass relation and maximum mass of white dwarf progenitors
  Monthly Notices of the Royal Astronomical Society, 1997
• A spectroscopic determination of the mass distribution of DA white dwarfs
  The Astrophysical Journal, 1992