The position of the most
likely host galaxy, VHS7, is highlighted on the plot.
Although the team has stared into the repeating FRB's patch of sky using several telescopes, they have yet to locate
a likely host galaxy.
Not exact matches
GOOD NEIGHBORHOOD The most
likely galaxy to
host habitable planets might be a giant elliptical such as ESO 325 - G004 (pictured, center), which is about 450 million light - years away in the constellation Centaurus.
That grim scenario has become more
likely based on a new survey of
galaxies hosting active black holes at their centers.
Because such black holes are most
likely to exist at the cores of
galaxies, a close enough look at a quasar should usually reveal the
host around it.
The
likely scenario in which this could have happened is if the
galaxy hosting the black hole experienced mergers or collisions with other
galaxies through its evolutionary history.
Portegies Zwart hopes to test his simulations by predicting which of the four YODECs in our
galaxy is
likely to
host a midsize black hole, which could be detectable via a bright X-ray signal.
The astronomers determined that this
galaxy's rapid star formation was
likely triggered by a close encounter with its slightly smaller companion, which already
hosts about 35 billion solar masses of stars and is increasing its rate of starburst at the breakneck pace of 540 solar masses per year.
Stars tidally stripped from their
host galaxies are the most
likely culprit, rather than unknown primordial
galaxies.
Such a shortfall is particularly prominent in luminous infrared
galaxies (LIRGs), which have high star formation (and thus CCSN) rates and
host bright and crowded nuclear regions, where large extinctions and reduced search detection efficiency
likely lead to a significant fraction of CCSNe remaining undiscovered.
«If they are supernova explosions, then their properties are more extreme than we have ever observed before, and are
likely connected to the central environments of the
host galaxies.»
FRB 150807, which the researchers believe most
likely originated from a
galaxy named VHS7 located between 3.2 and 6.5 billion light - years from Earth, was seen to be weakly distorted by material within its
host galaxy.
Astronomers at LCO then used the GLADE catalog (Galaxy List for the Advanced Detector Era) to identify
galaxies in this region of the sky and then applied an algorithm to identify which of these
galaxies would be most
likely to
host a kilonova based on properties such as their distance and luminosity.
Because of their distance from the
host galaxy, the ghostly green structures might have taken tens of thousands of years to light up after the quasar outburst, and would
likely fade tens of thousands of years after the quasar itself comes to an end, according to astronomers.