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U Sco 2010 outburst: observational evidence of an underlying ONeMg white dwarf
stars: individual: USco –novae, cataclysmic variables
2011/10/12
This paper presents U Sco nebular spectra collected in the period March-May 2010 after the binary outburst on Jan 28, 2010. The spectra display strong [Ne V] and [Ne III] lines that can be used to com...
Stark Broadening of Carbon and Oxygen Lines in Hot DQ White Dwarf Stars: Recent Results and Applications
stars: atmospheric parameters – broadening: Stark
2011/10/9
White dwarf stars are traditionally found to have surface compositions made primarily of hydrogen or helium. However, a new family has recently been uncovered, the so-called Hot DQ white dwarfs, which...
Convective overshooting in White Dwarf and ZZ Ceti stars
Convective overshooting White Dwarf ZZ Ceti stars
2009/6/10
Convective overshooting in White Dwarf and ZZ Ceti stars。
The evolution of intermediate mass stars from the main sequence to the white dwarf stage
mass stars white dwarf stage main sequence
2009/6/10
The evolution of intermediate mass stars from the main sequence to the white dwarf stage。
The evolution of iron white dwarf stars。