- The
Canis Major Overdensity (CMa
Overdensity) or
Canis Major Dwarf Galaxy (CMa Dwarf) is a
disputed dwarf irregular galaxy in the
Local Group, located...
- universe,
exceeding the size of the Huge-LQG by
about a
factor of two. The
overdensity lies at the Second,
Third and
Fourth Galactic Quadrants (NGQ2, NGQ3 and...
-
several small overdensities in the m****
distribution in the
Universe shortly after the Big Bang 13.61
billion years ago. Some of
these overdensities were the...
-
first one as it is that s**** that
travels the same
distance for all
overdensities before decoupling. This
radius is
often referred to as the
sound horizon...
- the
overall m****
balance of an LSB. The
centers of LSBs show no
large overdensities in stars,
unlike e.g. the
bulges of
normal spiral galaxies. Therefore...
- (2016-09-09), "Mapping the Most M****ive
Overdensities through Hydrogen (MAMMOTH). II.
Discovery of the
Extremely M****ive
Overdensity BOSS1441 at z = 2.32", The Astrophysical...
-
million light-years in extent. It is
currently unknown whether LABs
trace overdensities of
galaxies in the high-redshift
universe (as high
redshift radio galaxies—which...
- Arm.
Researchers have
found a
marginally significant arm-like
stellar overdensity close to the
Local Arm,
identified with the HMSFRs,
especially in the...
- The
Pisces Overdensity is a
clump of
stars in the
Milky Way's halo,
which may be a
disrupted dwarf spheroidal galaxy. It is
situated in the
Pisces constellation...
- with a size of 350 kpc. It has four
quasars embedded within it and a
overdensity of Lyman-Alpha
emitting galaxies. The four
quasars embedded within the...
