Andromeda galaxy warp Guhathakurta and Szubinski

VORTEX of FORCE

By Henryk Szubinski

and GUHARTHAKURTA

The Andromeda galaxy is going through a change into a barred type spiral galaxy

problems of the basics of the data on any variance used with the definition of the general law or rotation as the accellerated types of values that are responsive to the full values of multiples in a related to interaction by static zone alterations of the RESISTANCE values and the universal activity of a accessance to force and the basics of the rotational moment in a minimal displacement by variance of the full values of the motion in non stop vectorisations where the whole formats of their basic related to the definitions of the observations of the Andromeda and the usage of vector BITS to define the force of the motion similarity as based on the data that the whole section of spacetime is displaceing into a vortex of values in which the general basis for force is discovered..

The data on the sudden vanishing of the force and the related to values of the full implications of the values being reduced in synch with the reductions of displacability of the related to specifics so that the level reversal defines the expansion of the start field value

start field =exp ( reversal S-1)

related to displacement S-x

reductions of synch

S-x (S-1)=UPP

= multiple set equations of a vector UPP

multiple universes basic law of motion upwards that the no go zone down in seperation is economical and communicative both not being in the parameter described

basically the GLOBULAR cluster brightness as the edge on values will be faster in motion than the core value that relates a conservation of force to its centrality by the relativity of a LINK to the displacement of the force boosting whereby theese values are conserved in a type TUBULAR relation of BARRED relations much like a surfer in a tube to stabilise the wave effect:

basically the GLOBULAR cluster brightness as the edge on values will be faster in motion than the core value that relates a conservation of force of one surfer in one vector direction

but related to another surfer

to its centrality by the relativity of a LINK to the displacement of the force boosting whereby theese values are conserved in a type TUBULAR relation of BARRED relations much like a surfer in a tube to stabilise the wave effect:

basic boosting on the conservations of globular clusters in motion multiples here and there:

basically the illustration of the dimensional order of the surfer in type 1,2,3 dimensional progression to proove that the surfer is involved in a twist with the foreground and background of the BARRED tubes shows that both cannot occupy the same dimensional order

Basic type 1,2,3 H2O complex

responsive vector motion in both vectors as opposed vector directions is non existance of this rule of action &/or reaction

meaning that in basic the Newtonian mechnics of action and or reaction is divided into surfer positions of multiple GO types and their NO GO types as the usage of static force in Newtons that can do any manouvre by;

1) the  2 vectors against the 3D

2) the 2 surfers as in opposite vectors without symmetry

3) the 2 surfers as in compensated reality of the 2 warp tubes:

SANTA CRUZ, CA  Astronomers have obtained new evidence of an extreme warp in the stellar disk of the Andromeda Galaxy (also known as M31), our nearest galactic neighbor. The findings are being presented by Puragra Guhathakurta and Philip Choi of the University of California, Santa Cruz, and David Reitzel of UC Irvine at the American Astronomical Society meeting in San Diego, CA.

Previous studies had suggested the presence of a warp in the outer parts of Andromeda’s stellar disk. The new findings appear to confirm those observations and suggest that the warp in Andromeda may be the most extreme cases of a warped stellar disk ever observed in a spiral galaxy. Possible causes of the warp include interactions between Andromeda and its smaller satellite galaxies.

Many spiral galaxies, including the Milky Way, appear to have warps in the outer reaches of their stellar disks. The rotating body of stars and gas that characterizes a spiral galaxy is generally flat, but the outer regions may deviate from the plane of the disk, like an old record album exposed to too much heat. The warp tends to occur at the outer edges, while the inner part of the stellar disk remains flat. These warps are very difficult to demonstrate conclusively, however, because the outer portions of the stellar disk are extremely faint compared to the bright central region.

“The faint outer parts of the galaxy are more susceptible to warping because they are less strongly bound by the gravitational forces that keep the disk in a plane, and they are also more susceptible to the influence of neighboring galaxies,” Guhathakurta explained.


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The Andromeda Galaxy is a good candidate for studying a warped stellar disk because the plane of its disk is inclined toward the Earth at an angle of about 77 degrees (an inclination angle of 90 degrees would give a perfectly edge-on view of the disk). The inclination of Andromeda’s disk gives it an elliptical shape in the sky.

The new findings are based on two distinct sets of observations by Guhathakurta and his coworkers. The first set of observations was obtained using a large-format digital camera on the 0.9-meter Burrell Schmidt telescope at Kitt Peak National Observatory in Arizona. The images showed that the inner part of Andromeda’s stellar disk looks like a perfect ellipse, but in the extreme outer parts it starts to deviate. The warping gives the galaxy a slightly S-shaped appearance, with the outer edge tilted above the plane of the disk on one side and below it on the opposite side.

Older observations using photographic plates had suggested the same thing, but the features are so faint that they were at the limit of photographic detectability and were obscured by artifacts on the plates, Guhathakurta said. Modern digital cameras are far more sensitive than photographic plates, although they cannot yet cover as wide a field of view. In order to image the entire stellar disk of Andromeda, which covers an area of the sky several times the size of the full moon, the researchers had to take multiple images of adjacent areas of the sky and fit them together into a mosaic.

“The S-shaped pattern is very clear in the digital data. If you look at the digital images and the photographic work side by side, you can see the same thing, but you can also see why the photographic data was not very reliable,” Guhathakurta said.

The researchers also obtained additional evidence suggesting that the degree of warping in Andromeda’s stellar disk may be especially dramatic. This second set of observations was the unanticipated by-product of an unrelated study of stars outside the disk of the galaxy. Spiral galaxies consist of two components: the stellar disk and a ball-shaped collection of stars called the spheroid. The stars that populate the spheroid and the disk have very different properties. But Guhathakurta and Reitzel found stars with the properties of disk stars in a location far removed from the disk.

“We were trying to get as far away from the disk as possible to pick out stars belonging purely to the spheroid, and we had calculated the probability of finding a disk star where we were looking was much less than 1 percent,” Guhathakurta said.



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