The 9.8 years orbit results quite eccentric (e = 0.57), as typical for... ▽ More We have performed RV monitoring of
the components of the binary system HD 106515 over about 11 years using the high resolution spectrograph SARG at TNG.
Abstract: We have performed RV monitoring of
the components of the binary system HD 106515 over about 11 years using the high resolution spectrograph SARG at TNG.
Not exact matches
Most scientists are sure that in the centre
of our galaxy there is a supermassive black hole; there are
binary systems where one
of the
components is most likely a black hole.
Observations
of the explosions
of white dwarf stars in
binary systems, so - called Type Ia supernovae, in the 1990s then led scientists to the conclusion that a third
component, dark energy, made up 68 %
of the cosmos, and is responsible for driving an acceleration in the expansion
of the universe.
One
of the
component stars
of the
binary X-ray
system Cygnus X-1 is a black hole.
Alpha Centauri is a multiple - star
system, with its two main stars being Alpha Centauri A (α Cen A) and Alpha Centauri B (α Cen B), usually defined to identify them as the different
components of the
binary α Cen AB.
Together, the bright visible
components of the
binary star
system are called Alpha Centauri AB (α Cen AB).
Finally, noncoplanarity between the
component stars
of a
binary system should not have a significant impact on the stability
of close - in planetary orbits around each star (Alan Hale, 1994).
The primary
component in the
system is a spectroscopic
binary with the stellar classification
of B2 IV, matching the spectrum
of a blue - white subgiant star.