GIC COLLIDING GALAXIES GALLERY ANTENNAE THE FISH HAMBURGER CARTWHEEL DUSTING SILHOUETTE STEPHAN'S WINGS BORIS NGC 3314 NGC 6745 NGC 6872 NGC 5426 NGC 1232 UGC 10214 M74 COMET LINEAR HOW TO MAKE A LONG TAIL SUPPORT canopies.htm integral.htm intruder.htm antenna.htm motors.htm arms.htm jet.htm LENTICULAR NGC 1409 NGC 4650 ARP 102 COLLISION AFTERMATHS ANDROMEDA TRIANGULUM NGC 2997

COLLISION IN PROGRESS Ngc 3314 - A spiral cleaving into an edge-on, has caused lineal striations (upper left), a chopped arm (right of center), smooths, and other telltale clues including two blue doppler shifts in the spiral. Click on thumbnial for complete analysis.

POLAR RING GALAXIES

The next
two galaxies
on showcase are very
blurry, rather unhandsome,
but tehcnically revealing. Skip
over them if the images do
not turn you on

POLAR RING GALAXY NGC 1409/1410

The
smaller
(spiral) galaxy
is in the foreground, the
(larger) lenticular is in the rear
of the colliders



This dusty
pair of colliders
has a string between of an
entirely different kind than 'integral'. It
has been suggested the string is a mysterious form of
gravity stream but methinks not. The small upper galaxy
has a rudimentary form distintly seen in 'starburst'
class galaxies such as Ngc 1512, the lower object
has a twirling lenticular form distinctly
like that of Ngc 3718 even to
the curling end
waves.

The thin
strand starts
behind the starburst
and now behind the lower galaxy
seems to have passed through it, or, the
lower galaxy is rising forward being cut by the thin
strand if the thin strand has any kind of integral
strength. A wobble in the lower end of the strand
indicates rapid differential slipstream motion
there. The starburst form (linked as M94)
above, is also rudimentally seen in
one of the fish Ngc 2207 eyes







The
original
is very diffuse
and it is hard to coax
data out of it, however, here
are three coaxes showing enough datas
to make a point, that this is a lenticular
formation. Note again that the strand is
wobbled and irregular, with a small
buldge on the east side of the
center, meaning that this
area is very dynamic







POLAR RING GALAXY NGC 4650







It seems
there should be some
lenticular similarities between
Ngc 3718, Ngc 1409, and 4650, and, there are.
My guess is the long tag at the upper end of Ngc 4650, which
goes off screen, hooks back like a fishhook. Unfortunately
no good images of Ngc 4650 seem to have survived pre
release editing and so none are to be found
except Hubble's, at least, none
that show more than the
center 'polar ring'

The
lower thrust
can be said to be a
foot pad in a chaotic state

FOOT PADS (RINGS AROUND LONG ANTENNA) RESULTING FROM COLLISIONS

LENTICULAR GALAXY NGC 3718



GALAXY COLLISIONS ARP 102



GALAXY COLLISIONS NGC 4038



Note
the above
three (Ngc 3718),
(Arp 102), and (Ngc 4038),
all have a foot pad (rings around
the end of a long antenna). Bodes galaxy
has a profound geometric foot pad with ring
nearby off the end opposite to the
current position of bare M82
which is departing a
collision with
Bodes

BODES GALAXY HAS GEOMETRIC FOOTPAD IN CLOUDWALL



RESIDIUALS CLUMPED UNDER AND BEHIND BORIS

At M51,
underneath
and behind Boris
are coherent forms described
as perhaps residues of former galaxies
however the residues also have the form of
a footpad, which, if correct, indicates
that 'footpads' commonly result
from collisions



STARBURST CLASS GALAXY SHAPE





STARBURST CLASS GALAXY SHAPE IN NGC 1409/1410







Stereo
reveals we
are looking at
this object at more
end on, the right blue limb
far closer to the camera. It means
the object has been strenuously torqued
twisting the two main arms into sharp
bi-lateral symmetry mode quite
outstanding in terms of
usual bi-laterals
in galaxies

STARBURST CLASS GALAXY SHAPE IN M64

Another
starburst
shape, very diffuse,
hazy, spread out, is seen in Ngc M64

LENTICULAR TWIST GALAXY NGC 4656

A lenticular
with twirling wrap
around twists is Ngc 4656. A
diffuse irrgular clump (upper right) also
has twists twirling clockwise but at an opposite
polar vector, indicating a common angular momentum
source is cause of these lenticular twists. And so it can
be logically equated that the small bullet (upper
right) imparted the lenticular twists to the
larger galaxy and stretched it. Or, else,
The lower end of the larger galaxy
glanced by the small clump
causing the two vectors
of polar opposite
twists one in
each by
corkscrewing
in sheer momentums.
In any case, the small clump
must be a remnant after a major collision,
its original hot bright core is gone, perhaps attached
to the lower upper left of the lenticular as a long oval incise

OVBERLAPPING PAIR NGC 5090

There is
some discussion
in abstracts et al as to
if this is an overlapping pair or
two galaxies engaged. Interest in overlapping
pairs is in attempting to determine how much dust in
the overlap obscures the radiance of an overlapped galaxy.
It is hard to tell (in mono) often, if a pair is engaged or is
overlapping. In stereo the following pair seem not
engaged and overlapping, the spiral to the fore
overlapping a rearground elliptical. High
enhancement has not revealed any
connection between the
spiral to the
elliptical
and stereo
reveals the
elliptical is
slightly back. Any
engagement is extremely
marginal, the rear edge of the
spiral is obscured by elliptical haze

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