Not exact matches
Using simulations
to measure how radiation from one
galaxy influenced black hole formation in the
other, the researchers found that the neighboring
galaxy could
be smaller and
closer than previously estimated.
«Many of the stars in the bridge appear
to have
been removed from the SMC in the most recent interaction, some 200 million years ago, when the dwarf
galaxies passed relatively
close by each
other.
Other so - called hypervelocity stars
are thought
to have
been boosted
to their high speeds by
close encounters with our
galaxy's supermassive black hole (see Hypervelocity stars: Catch them while you can), but this star
is too young
to have travelled all the way from the centre of the Milky Way.
The theoretical engine of this growth turns out
to be complex: New
galaxies get pulled in and stretched around the halo like strings of spaghetti, maintaining the signature of their independent origin;
galaxies closer to the central bulge get mixed up with
other old structures, losing the hallmarks of their original form.
Ghost - like particles that
were first created in the instant following the Big Bang, antineutrinos and their partner neutrinos travel at
close to the speed of light and
are notoriously difficult
to observe as they move through space, passing through planets, star systems, and
galaxies with scant interactions with
other forms of matter.
Since the 1960s Margaret and a few
others have
been collecting examples of
galaxies and quasars in seemingly
close proximity
to one another.
These two
galaxies are close companions and it
is likely that a recent
close encounter has left both
galaxies looking very similar
to each
other.
The reasonable assumption
is that we do not live at a special time, so the
galaxies in the cluster must have always
been close to each
other.
«This contrasts with the recent X-ray determinations of (
close to) maximal black hole spin in
other [similar
galaxies] based on relativistic smearing of the iron profile,» the researchers wrote in the study, which
was published online today (July 29) in the journal Monthly Notices of the Royal Astronomical Society.
However,
other measurements taken by a team of researchers from the University of Strasbourg in France appear
to show that stars just outside of Triangulum II
are moving faster than the ones
close to the galactic center — which
were used by Kirby
to determine the
galaxy's mass.
Another result from the study
is that the jet structure in NGC 1275 significantly differs from the jet in the very nearby
galaxy Messier 87, which
is the only
other jet whose structure has
been imaged equally
close to the black hole.
The
galaxies in the two groups
are physically
close to each
other and the groups seem
to not
be moving relative
to each
other, so they
are often identified as a single
galaxy group.