GW170608 is
the lightest black hole binary that LIGO and Virgo have observed — and so is one of the first cases where black holes detected through gravitational waves have masses similar to black holes detected indirectly via electromagnetic radiation, such as X-rays.
Not exact matches
However, the team says the nebula's
light spectrum is different to that of a
black hole jet seen in a
binary system called SS 433.
Giant
binary stars, for example, typically produce
black holes lighter than the ones LIGO sees and too far apart to merge.
The team sifted through data from all the x-ray sources situated within 70
light - years of Sgr A *, searching for those that had characteristics of
black holes and neutron stars in
binary systems and found four sources within just three
light - years of the central
black hole.
Such events could include the mergers of
lighter binary black holes, of
binary neutron stars or of a
black hole with a neutron star.
In such a cluster, massive stars would sink towards the centre and, through complex interactions with
lighter stars, form
binary systems, possibly long after their transformation into
black holes.
Findings from this and two previous discoveries of
black hole mergers are providing the WSU scientists and colleagues at the Laser Interferometer Gravitational - Wave Observatory (LIGO) an unprecedented glimpse into the early universe and shedding new
light on how
binary black holes form.
But its announcement was delayed due to the time required to understand two other discoveries: a LIGO - Virgo three - detector observation of gravitational waves from another
binary black hole merger on August 14, and the first - ever detection of a
binary neutron star merger in
light and gravitational waves on August 17.
[Laughter] The
binary black hole system we detected was 1.5 billion
light years distant.