Not exact matches
We once thought that dark matter might be made up of large objects such as black holes or exotic types of
faint stars — neutron
stars or
white dwarfs — that are nearly invisible to our telescopes.
But von Hippel, Gilmore and their colleagues used the Hubble Space Telescope, and this allowed them to identify and measure the temperature of
white dwarfs as
faint as 25th magnitude, which is about 100 million times
fainter than any
star visible with the naked eye.
Maybe it was just large accumulations of dim but familiar objects, like extremely
faint red
stars or
white dwarfs, some astronomers speculated.
«Our final image should show us a companion 100 times
fainter than any other
white dwarf orbiting a neutron
star and about 10 times
fainter than any known
white dwarf, but we don't see a thing,» team member Bart Dunlap, a graduate student from the University of North Carolina at Chapel Hill, said in a statement.
«You can see bulges in distant galaxies, but you can not resolve the very
faint stars, such as the
white dwarfs.
During that night, the scientists were able to measure the changing Doppler shift of the
star NLTT 11748 as it orbited its
faint, but more massive,
white dwarf companion.
When this happens, smaller
stars expand into what astronomers call red giants, then shrink into
faint white dwarfs, according to NASA.
A 1997 paper by astronomers (Henry et al) associated with the Research Consortium on Nearby
Stars (RECONS) suggests that the sample of stars known to lie within 10 parsecs (32.6 ly) of Earth is «woefully incomplete,» particularly in faint red (M) dwarfs and «white» dw
Stars (RECONS) suggests that the sample of
stars known to lie within 10 parsecs (32.6 ly) of Earth is «woefully incomplete,» particularly in faint red (M) dwarfs and «white» dw
stars known to lie within 10 parsecs (32.6 ly) of Earth is «woefully incomplete,» particularly in
faint red (M)
dwarfs and «
white»
dwarfs.