As the white dwarf accretes material from the nearby star, it's possible that could explode as a type la supernova.
Not exact matches
The
white dwarf accretes material from the companion star, then at some point, it might explode
as a type Ia supernova.
Building on past observations of the
white dwarf called SDSSJ1043 +0855 (the dead core of a star that originally was a few times the mass of the Sun), which has been known to be gobbling up rocky material in its orbit for almost a decade, the team used Keck Observatory's HIRES instrument fitted to the 10 - meter Keck I telescope
as well
as data from the Hubble Space Telescope to measure and characterize the material being
accreted by the star.
«Spectroscopic observations of the
white dwarf allowed us to measure the abundances of the rocky material
as it is being
accreted and filtered through the star's atmosphere in real time,» Melis said.
If the
white dwarf accretes enough material to reach the Chandrasekhar limit, the maximum mass of a stable
white dwarf star (1.4 solar mass), it will likely explode
as a Type Ia supernova.