What Causes Elliptical Galaxies to be Elliptical?

  • Thread starter shounakbhatta
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In summary, the spiral arm patterns in galaxies are not thought to be due to a stationary spiral pattern, but rather are the result of mergers and gravity.
  • #1
shounakbhatta
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Hello,

I read that the density wave theory makes up the shape of the spiral galaxies look spiral? Is there any specific reason for elliptical galaxies to make the shape of a ellipse?

Thanks.
 
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  • #2
http://en.wikipedia.org/wiki/Elliptical_galaxy

The above may help. Since they seem to form from the merger of two or more galalxies, the original spiral shape gets lost and the ellipsoid result seems to be the natural shape resulting from gravity and angular momentum.
 
  • #3
Thanks for the information. I read through wikipedia. It says mostly they are formed by mergers of other galaxies.
 
  • #4
shounakbhatta said:
Hello,

I read that the density wave theory makes up the shape of the spiral galaxies look spiral?
This theory seems to have been recently falsified:
http://arxiv.org/abs/1105.5141

"Observational Evidence Against Long-Lived Spiral Arms in Galaxies"
Kelly Foyle, Hans-Walter Rix, Clare Dobbs, Adam Leroy, Fabian Walter
(Submitted on 25 May 2011)

Abstract: We test whether the spiral patterns apparent in many large disk galaxies should be thought of as dynamical features that are stationary in a co-rotating frame for > t_{dyn}, as implied by the density wave approach for explaining spiral arms. If such spiral arms have enhanced star formation (SF), observational tracers for different stages of the SF sequence should show a spatial ordering, from up-stream to downstream in the corotating frame: dense HI, CO, tracing molecular hydrogen gas, 24 micron emission tracing enshrouded SF and UV emission tracing unobscured young stars. We argue that such a spatial ordering should be reflected in the angular cross-correlation (CC, in polar coordinates) using all azimuthal positions among pairs of these tracers; the peak of the CC should be offset from zero, in different directions inside and outside the corotation radius. Recent spiral SF simulations by Dobbs & Pringle, show explicitly that for the case of a stationary spiral arm potential such angular offsets between gas and young stars of differing ages should be observable as cross-correlation offsets. We calculate the angular cross-correlations for different observational SF sequence tracers in 12 nearby spiral galaxies, drawing on a data set with high quality maps of the neutral gas HI, THINGS), molecular gas (CO, HERACLES) along with 24 micron emission (Spitzer, SINGS); we include FUV images (GALEX) and 3.6 $\mu$m emission (Spitzer, IRAC) for some galaxies, tracing aging stars and longer timescales. In none of the resulting tracer cross-correlations for this sample do we find systematic angular offsets, which would be expected for a stationary dynamical spiral pattern of well-defined pattern speed. This result indicates that spiral density waves in their simplest form are not an important aspect of explaining spirals in large disk galaxies.
 
  • #5
So where do we stand?
 

1. What is the main factor that causes a galaxy to have an elliptical shape?

The main factor that causes a galaxy to have an elliptical shape is the lack of ongoing star formation. This means that the galaxy lacks young, hot stars and is instead dominated by older, cooler stars. The motion of these stars creates an overall elliptical shape.

2. Can external forces, such as collisions or interactions with other galaxies, cause a galaxy to become elliptical?

Yes, external forces such as collisions or interactions with other galaxies can cause a galaxy to become elliptical. The gravitational pull from another galaxy can disrupt the original galaxy's structure, causing it to lose its spiral arms and become more elliptical in shape.

3. How does the age of a galaxy relate to its shape?

The age of a galaxy plays a significant role in its shape. Elliptical galaxies are typically older than spiral galaxies, meaning they have had more time for their stars to age and cool. This is why they lack the hot, young stars that give spiral galaxies their distinctive shape.

4. Are all elliptical galaxies the same shape and size?

No, not all elliptical galaxies are the same shape and size. Just like with other types of galaxies, there is a wide range of shapes and sizes within the category of elliptical galaxies. Some may appear more spherical, while others may be elongated or flattened.

5. Can elliptical galaxies ever change shape or become spiral galaxies?

It is possible for elliptical galaxies to change shape or become spiral galaxies, but it is rare. This can occur through interactions with other galaxies or through the merger of two or more galaxies. However, these events are not common and most elliptical galaxies will maintain their shape throughout their lifetime.

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