(GIC) HERCULES GALAXY CLUSTER CIRCLE SOFT OVAL UFO'S SUPER galaxy cluster images Perseus A giant elliptical galaxy in collision LEO TRIO PERSEUS EEL TAIL

A SEARCH THROUGH DSS IMAGES FOR OTHER COHERENT OBJECTS IN GALAXY CLUSTERS PULLED UP BLANK, EXCEPT FOR TWO OBJECTS IN THE HERCULES CLUSTER, AND OBJECTS IN A CLUSTER WITH NGC 3190.

GIANT RING IN THE HERCULES GALAXY CLUSTER

This is a large diffuse thin ring, which suspiciously looks like a ring from a telescopes light strike, but, it is suspiciously riddled with clues saying otherwise.

   

   





If the rim of the ring has rotated in more than one vector through time, it explains why the four cardinal points crossing the rim are slewed in opposed directions. Another clue are faint inner ring residuals as second smaller circumpherences indicating this was once (if real) a brighter more coherent great object. The impression is this structure is old. The dark hole near the center, expect as an image flaw, has texture within, suggesting it may instead be a dark or light inhibiting object. Dark holes are not uncommon in deep space.

The bright sputs with 4-way star points lower right is an overbright star from the Milky Way.



Dark holes as image flaws can look like this - chicken pox riddle an image of the Perseus galaxy cluster.



A solid nail hole in an image of Ngc 1608.



THE HERCULES SOFT LANDING OVAL

The soft landing site island oval is very weak, very dim, but here it is intact. The left edge of the Hercules oval is visible upper right.

     



GALAXY CLUSTER ABELL 2390

       

           

   

If you overlay the two above images together by merging them by eyesight new important details are revealed, for instance huge circular rounds pillow forth like gear housings in complex differentials, the huge rounds perhaps the donkeys having enough storehouse of low radiant mass to satisfy the needs of gravity in keeping galaxies clustered together in small local herds.

A Dss 2nd generation blue image of Abell 2390 galaxy cluster shows a great deal of clumping of small conglomerates of sundry deep space matter.



A Dss 2nd generation red image of Abell 2390 galaxy cluster shows a more homegenously distrubuted deep space sundry matter field.



A 1st generation Dss image of Abell 2390 galaxy cluster shows a more patterned backdrop with many local cyclonnic swirls, and rivers of entropy flowing in streams. The predominent sundry mass distribution is in the left side of the field, in contrast to the 2nd red and 2nd generation blue images where the greater (brighter) sundry mass density is to the left.



THE LEO TRIO (THREE GALAXIES)

That deep space objects found in images highly enhanced can have real meaning is well suited in being illustrated by these next two views of galaxies M65 and M66, both views by entirely indendent telescopes and photo capture methods, both show a large concentrated sphere of denser (or hotter) matter in the inter medial space between the two galaxies. It means without question that the gas ball is out there between the two galaxies.

IMAGE SOURCE 1









IMAGE SOURCE 2







Notice that both source images (1) and (2) show streamers trailing in deep space turbulence between the dim center picture gas ball and the upper galaxy, no streamers or tendrils are seen leading to the lower galaxy. The implication is that the upper galaxy has shared space in an encounter with the giant gas ball. A luminant bridge between two galaxies which shared space is seen in a color photo of M81 and M82 (Bodes galaxy and the 'cigar' galaxy).

A Dss plate enhanced by Histogram Equalize also shows turbulence between M66, the turbulence ends at the lower end of the giant gas ball which remains un-illuminated in the Dss view.







Stereo (go cross eyed to see the stereo) reveals that M66 is very far back in deep space, Ngc 3628 to the right seems closest to the camera although it is not easy to tell if Ngc 3628 is in forespace in front of M65 below in the picture.






In the AAT image of the Leo Triplet, most of the deep space background has been scraped away from the image by photo processes so no turbulence or media densities between galaxies can be seen.

DEEP SPACE SHADOW OBJECTS AT NGC 3190

A dss photo of galaxy Ngc 3190 is interesting. The 1st generation photo shows nothing. The 2nd generation plate (red) also shows nothing of interest. Because they are bland, there is no reason to show the 1st and 2nd generation images. If you need them, the Dss jukebox has them.

The 3rd plate (2nd generation blue) is filled with items of intrigue causing halts to translate into concentration. For instance a large dark hole is in the 3rd plate near the bottom just past center. Another dark hole (smaller) is further to the right.









An object which looks in every way like a UFO is near the group's upper left elliptical galaxy. That elliptical galaxy has two bright prongs jutting westward, these prongs are not seen or even indicated in the other two plates. All in all, blue has a lot to say about the deep space region housing galaxy Ngc 3190. Which is interesting, because deep space in Dss 2nd generation blue images usually are homogenously bright and bland.

UFO's near an ellipical galaxy. Neither the wings (prongs) nor the time top have instant explanation as plate flaws or otherwise.







Actually, the time top looks in many ways like a gordian knot colliding galaxy (writhed and tangled) very dim. View the image pair in stereo by gently going cross eyed to see that the time top is a gordian knot galaxy object, not rain on an astronomer's parade.





   

How far can you stretch the elastic band. At almost subliminal reliability, the verticle winding on the right looks like it could be a captured lenticular galaxy. But like I say ... s t r e t c h.

In fact, the time top looks like a very faint spindle galaxy.

You know that I am taking terrrrible risks to my burgening career as an easy going free will thinker by presenting UFO's in a Dss images as perhaps legitimate.

Give a one-second three-palm handclap for the author (myself). Large images like these above are hard to factor and interpret, and even harder to fit into display schemes. I think I have done all right, concidering the challenges.

LARGE DARK HOLES

Two giant dark holes. Both have texture within and the left a seeming tadpole tail extension vectoring away, and the left dark hole has a bright center, all suggestive of coherent objects rather than drops of developing solution on the photographic plate. Perhaps 'rain drops are falling on my lens' is a possibility - perhaps dew drops, no photoshoot if it is raining - tautology.





Concentric overplapping crescents do not appear until the image is enlarged to its maximum size, (in which all small details are gone in too-stretched opened up resolution which is typical of Dss 1st generation images enhanced by Histogram Equalize which rarely can be used in full size display). Instead in this case (2nd generation blue) the unusual character of overlapping density distribution crescents emerges even more so from the very dim, deep space, low radiant, sundry media backdrop, as recorded in the Dss image, when shown full size.



A colored image - fast travelling whack slam click on the internet late one afternoon, source unknown - highly enhances into deep space drifts between the galaxies.



For academia enthusiasts, here is some record. The above Ngc 3190 images are another group within the Leo Triplet umbrella, this group of four galaxies known - besides as the second 'Leo Triplet' - also as Hickson 44, which contains Ngc 3190, Ngc 3187, Ngc 3185, and Ngc 3187. Here (click) is a road map nipped from the internet, written atop a Palomar image.

Stretched galaxy Ngc Ngc 3187 (left) falls within my 'Antenna' class and is features, along with other stretch galaxies, at the antenna page.


THE GREAT BRAIN DRAIN SEARCH

Incidentally, the blk&wt (above left), and color views below, may be the best versions of Ngc 3187 you will see at this time (Nov 2001). Both views were enhanced by myself from available data seen faintly in images further above in this page.

I searched Google for Ngc 3187 and at the sixth bottom row page link began to feel a great brain drain and quit. If you wish to grope the state of the art in astronomy regards more obscure objects such as Ngc 3187, do a Google search and see the image quality consistently throughout.

Yipe. See, my interest amongst many is how a galaxy gets stretched like this and the only way I can investigate is to compare stretched galaxy images looking for clues. Today, I learned no new clues because Ngc 3187, pristine, large, clear, brillient, was not found on the Internet by me by the great brain drain search.

For instance, Ngc 3187 has a noticeably long eel tail, unusually so amongst galaxies commonly known. The original, from which the following color views were brained, shows nothing of the eel tail.

Stretched galaxies include items such as Ngc 6872 and Ngc 2442.

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

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