Today the central star is of mag 16.6 and a high temperature of some 60,000 K, which will probably cool down
as a white dwarf over the coming tens of billions of years.
Not exact matches
Kailash Sahu and colleagues at the Space Telescope Science Institute in Baltimore, Maryland, measured bending light from
white dwarf Stein 2051 B
as it moved in front of another star
over two years.
As a
white dwarf draws off hydrogen - rich material from a binary companion
over millions of years, Gilfanov says, it experiences a steady process of nuclear fusion on its surface that gives off tremendous amounts of radiation.