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    rills in interspace backdrop     Super Nova sn1987
    See also cyclonnic swirls in small galaxies

HERE COMES THE 'GLOMMER' GALAXY CYCLONNIC SWIRLS AND DARK/LIGHT LENSES IN LMC

What is seen (original)
what wasn't seen (enhancements)







Dominant
color tone
enhancements break
up the object into two divisions,
(the LMC enhances strongly in yellow and green),
(the rest enhances strongly in blue and red)

Enhancements
have revealed two
components of interest -
a dynamo motor thrusts from
the right helm ending abruptly in
dark space, and a lateral slash or jet
of bright clumps, very off center, crosses
the top to the left where an incise abruptly
changes media around a cavity with sharp edges.
These above images are powerful in revealing
a wormgear or lookalike thrusting out
far into the right outer flank
from the motor

SMALL GALAXIES COLLISION IN PROGRESS - MEET THE 'GLOMMER' GALAXY

I half
suspect that
the wormgear lookalike
is the dimmed core remnant of
another irregular galaxy (about half
the size of LMC) which is sliding over
the top of LMC from rear left the other end
of the colliding galaxy the wormgear, the
overcover of the other galaxy glommed
to the top of LMC is the cause
of the noticably sharp
incise. In reverse
point of view
the incise
is original
LMC media which
is less mixed and chaotic
than is the media of the glommer,
for this reason the incise seems precise.
To achieve this precise degree of incise means the
glomming galaxy is actually moving forward from behind,
the corethrust and motor already progressed far forward the
upper left is still rearward just now cutting into the LMC
landscape causing incise cavity. The glommer galaxy
has to have a radial axis that travels foreground
lower right (middle of the above images)
to the far rearground upper left
where the string of hot
star clumps ends. In
this case, all of
the hot star
clumps are
directly
in cause by
the incoming glommer
galaxy moving forward intermixing
with original LMC matter, in which case the
'glommer's velocity is slow allowing enough time for
percussive intermixes to occur. (It may be that
extra fast motion(s) are needed to fire
up the hot star clumps - I guess
slow velocity for hunch
reasons only)



The
cyclonnic
swirls sweeping out
in ghostly arcs into the right
field may be skeleton residues of what
were once arms, only traces of the
original angular momentum paths
taken by the arm(s) now are
seen. It seems the
skeleton arm(s)
belong to
Glommer

To be
punctually
correct, it has to
be said that LMC may be
moving into the body of the
Glommer which is the slower
mover, in converse to the
motions suggested
in the above
paragraph

The
insight
forecluding
collision came
about very quickly. I
had just done an enhanced window
for this view and the moment superimposed
the overlay image combination revealed the
wormgear thrusting out in front of the motor.
How can this be, was my first response, what the
heck is that wormgear doing there, the second resonse
a moment later is wait a minute this is another galaxy!

A STUDY OF DARK/LIGHT IMAGE AREAS, AND PRISMATIC REFRACTIONS

Image rotation
shows cyclonnic motions
(swirls) in numerous diffuse ways
around the dynamo. The lateral jet (now down
the right image-edge), though hard to see without will
power, seems more to be merely an irregular
edge to the galaxy



A large
size vertical
view in mono shows more
of the trail of roiled turbulence
up the right edge. As well, vertical strings
made of stars shoot in parallel out through the dynamo
into space in the picture's bottom left. As well, many small
rosettes made of stars pepper the LMC face, and horizontal
lines some made of stars in long strings, are in the
enhancement. The vertical roil down the right
edge is actually made of a string of
small rosettes that converge
in size from larger to
smaller in the
image bottom

DARK/LIGHT - AN EXTRAORDINARY PHENOMENON IS HIDING LIGHT

The
dark/light
phenomenon is really
there, all images of the LMC
show it to one degree or another.
The Tarantula Nebula is the spider
shaped white clump above right

NUMEROUS COHERENT SMALL RADIAL PATTERNS MADE OF STARS, SOME SEEMING TO BE STRAIGHT EDGES OF HEXAGRAMS, FILL THE AREA

A shin
plaster
rosette is
revealed in these
particular enhancements
immediately above, the rosette is
six sided and sits settled into the
left hand. In no way perfect,
nevertheless, there it is





Next, the
wormgear juts
out on its own





Another
shinplaster
rosette cluster, this
time two rosettes partially merged.
A similar configuration has been
spotted in a hot star field
in the Milky Way



Next,
dark/light
straight edges.
Long lines of sharply
contrasting medias, are noticable

PRISMS AND CYCLONNIC SWIRLS MADE OF COHERENT STAR PATTERNS

IMPORTANT IMAGE

The
vertical
slash in close
together converging
vectors is a trench
moiled in foam

PRISMATIC REFRACTIONS

Prisms
of refractions
in galaxies are not so
extraordinary, not as if hand made
by mighty migrating Egyptian engineers
building pyramids of cream puff from
galaxy matter. Clouds on Earth,
layered certain ways, become
highly precisely prismatic
when sunlight shines
through at certain
angles. You
all have
seen
prismatics
in concentric
radiant patterns in the
skies at one time or another in your life









The original is an Noao image, sourced here.

The same original LMC image has appeared at Apod.

CYCLONNICS (CIRCULAR FORMATIONS)

Cyclonnics
(circular formations)
are certainly a big thing in the
LMC. Here is a 'circular cyclonnic' around
an object captioned as the 'NGC 2014, Henize 55
in the Large Magellanic Cloud' by AA0



Images
of LMC showing
its full size seem combed
from the Internet any LMC image seen seems
cropped to show just central details or the tarantula. One
Noao image is a deep space view showing both LMC and SMC the content
so dim LMC is just a blur but info can be coaxed out of it by tweaking
the knobs of a graphic editor such that some semblence of full
size but not full illumination of LMC is possible

PRISMATIC REFRACTIONS IN STAR FIELD NGC 4214

CONCENTRIC CIRCULAR PYRAMID REFRACTIONS IN GALAXY NGC 253

THE 30 DORADUS STAR FIELD IN THE LARGE MAGELLANIC CLOUD (LMC)

AAT image of 30 Doradus and Super Nova 1987a





The 30
Doradus star
field, and within it the
center spread known as the Tarantula,
are the bright red/white tangle hoving above the
Large Magellanic Cloud galaxy up there toward the left.
An AAT photo close-ups, the 30 Doradus structure,
in which the super nova of 1987 called Sn1987a
is the bright round blare diagonally
to the lower right in the
AAT image

SUPER NOVA SN1987 BY RADIO TELESCOPE

Australia's new CSIRO radio telescope releases this image of super nova Sn1987a in the Large Magellanic Cloud, the image cheered in showing extensive new details captured for the first time at shorter radio wavelengths. The image released, is threadbare with a bright center (left view) compared to the amount of information the image actually contains.

And now for one of those hanky panky mystical mystery shows which sometimes happens in circumstances of great intrigue and no explanation. Next is a view enhanced several weeks ago by myself which shows tiny pinprick stars colonizing the edges of the bright radio bands.





The pinprick stars were spotted in this image, during a proof reading run.

The pinprick stars are in the image, no way a computer could have accidentally generated these. How they got in there (in the image) is the mystical mystery - I have no idea. I wish I knew how. It seems to me a way of photosnapping stars in pinprick scale is a lot better than the blaxing big beads telescopes normally get for any stars in number.

I have tried to recreate a new image showing the radio pinprick stars to no luck, I tried everything I could think of that might have caused the pinpricks to be revealed, the only thing 'try' achieved were better more textured views of the radio density bands, seen next.

SUPER NOVA SN1987 IN VISIBLE LIGHT

Click to see a Hubble Sn1987a original (which clearly shows the super nova in the left panel, and an enhancement clearly showing the surrounding galaxy murk in the right view.



Strong red color enhancement (plus gamma correction) shows extensive filamentation in the form of lineal and circular thin lines some in coherent patterns, riddling the fields of sundry matter.



More Sn1987a images are   here 1   here 2   here 3   here 4.

For name's
sake, the second
galaxy comprising LMC is called
'Glommer' because it seems to be glommed to LMC
like glucotomus glob, but, in fact, the collision is a by-pass,
two galaxies slicing and shearing past each other since both
galaxies are small, both are experiencing image change
and heat entropy re-distribution at a rapid pace

 

 

LARGE CYCLONNIC SWIRLS IN SMALL GALAXIES

TUBE SHAPED SMALL GALAXIES

THE REAL SHAPE OF SMALL DWARF (IRREGULAR) GALAXIES

Without spiral arms, instead small galaxies have a torpedo shape with a pronounced cyclonnic swirl jutting into space from one end.

Images which show the cyclonnic swirl cannot show if a similar formation occurs behind the galaxy in the rear side being blocked from view. The forefront view is revealing - if more than one galaxy has such shape then the shape is established as characteristic for at least some small galaxies.

Here next are two local neighborhood galaxies which have the shape, LMC (Large Magellanic Cloud), and Ngc 6822.

GALAXY NGC 6822

Hubble images source site.

Irregular dwarf galaxy Ngc 6822 seems to have a forethrusting cyclonnic similar to but less distinct than that of LMC

CYCLONNIC WHIRL IN LMC



CYCLONNIC WHIRL IN NGC 6822









A sequence of several different color tones each reveals its own presence of the cyclonnic swirls around the front end on a galaxy who's oriented view is tilted slightly to the right rather than full end on.

Also, there are small chains and links in neckalces made of stars in arcs and circles, a particularly strong star circle of small radius in the lower left of the frame. Star chains and necklaces are explored in globular clusters in this GIC page.

Next is a view of Ngc 6822 at larger scale.

Web site/display/designs/image enhancements - Greydon Moore World's largest cosmic teaching site - Ottawa 2001/2004         form   A & O 3 3