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Darkmatter Selfproofs |
SELFPROOF O504 - STARS AT A GALACTIC CENTRECURRENT COSMOLOGY MODEL
The
central parsec around Sagittarius A* contains thousands of stars.
Although most of them are old red main-sequence stars, the Galactic
Centre is also rich in massive stars. More than 100 OB and Wolf-Rayet
stars have been identified there so far. They seem to have all been
formed in a single star formation event a few million years ago. The
existence of these relatively young (though evolved) stars was a
surprise to experts, who expected the tidal forces from the central
black hole to prevent their formation. This paradox of youth is even
more remarkable for stars that are on very tight orbits around
Sagittarius A*, such as S2. The scenarios invoked to explain this
formation involve either star formation in a massive star cluster
offset from the Galactic Centre that would have migrated to its
current location once formed, or star formation within a massive,
compact gas accretion disk around the central black hole. It is
interesting to note that most of these 100 young, massive stars seem
to be concentrated within one (according to the UCLA group) or two
(according to the MPE group) disks, rather than randomly distributed
within the central parsec. This observation however does not allow
definite conclusions to be drawn on this point. (Wikipedia
6 Aug 2012)
MALTA COSMOLOGY TEMPLATE
- Every
blackhole in the Universe is within the gravitysheath of a larger
object. (see Argument 0336)
- Many blackholes are within the teelospheres of larger objects.
(see Argument 0337)
- Blackholes absorb teels from the teelosphere they are within which
alters the blackhole's measures of mass and energy. (see Argument 0338)
- A
stable blackhole within the teelosphere of a larger object becomes
understable due to the differential absorption of mass and energy
from the teelosphere. The stability of already overstable or
understable blackholes alters commensurately. (see Argument 0339)
- A
stable blackhole within a teelosphere, made understable through the
differential absorption of mass and energy, ejects more than it
absorbs until it returns to stability. The stability of already
overstable or understable blackholes alters commensurately. (See Argument 0340)
COMMENTARY
- The
Sagittarius A* blackhole is the understable hub of a teelosphere
that extends way beyond its disc of stars. The speed and density of
this teelosphere decreases with distance from the surface of the
blackhole per the Inverse Square Law. This means that within (say)
half a parsec of the surface the teelstreams in the teelosphere are
extremely dense and extremely fast. Any stars in this region are
both marshalled by the teelstreams and subject to a constant
absorption of teels from them.
- Because
the stars are constantly absorbing enormous quantities of very high
realspeed teels, they are extremely understable, as are the
particles they are made of. They are controlling their
understability by ejecting enormous quantities of teels and photons
but such is their rate of absorption that they can never stabilise
until the blackhole itself comes nearer to stabilisation.
- The
net effect is that these stars do not age. Per the Current Cosmology
Model, these are young stars but in practice they could be very old.
Such is the battering they are receiving that, their brightness
notwithstanding, they are probably quite diffuse and have a minimal
fusion activity.
- One
consequence of the battering they are receiving is that each of the
stars has its own extremely dense and extremely fast teelosphere
which functions as a defensive shield. This is why these stars are
able to cluster so closely together without either colliding or
gravitationally tearing each other apart.
CONJECTURES FOR FURTHER RESEARCH
- It may be that the number of stars clustering around the
blackhole is conditioned by the mass of the blackhole in the same
way that the number of electrons clustering around specific nuclei
is controlled.
- It
may be that the blackhole's teelosphere conditions the mass and
dimensions of the stars.
- It
may be that the markedly different nature of these stars, as
compared to those only a short distance farther out, is because
they are actually within the blackhole's teelocean.
- It
may be that, if the number of these stars is conditioned by the mass of
the blackhole, if one star in the cluster decays for any reason it will
be replaced by one of the stars from outside the cluster which is
then “rejuvenated” by its dense teel battering.
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