Picture of "very" blue galaxy, good place for super nova?

In summary, "Cosmic Map Reveals a Not-So-Lumpy Universe" is an article about a study that used a new method to map the distribution of matter in the universe, revealing a more uniform structure than previously thought. The study also included a picture of galaxy NGC 1398, which was discussed in terms of its velocity, star formation rate, and potential as a source of supernovae. The article also mentioned the possibility of finding astronomy databases for students to use for further research.
  • #1
Spinnor
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This story, "Cosmic Map Reveals a Not-So-Lumpy Universe",

https://www.scientificamerican.com/article/cosmic-map-reveals-a-not-so-lumpy-universe/

included an interesting picture of galaxy NGC 1398,

adamblock_ngc1398_1440.jpg.CROP.original-original.jpg


Also seen here,

http://www.slate.com/blogs/bad_astronomy/2014/12/22/ngc_1398_barred_galaxy_photo.html

Would this be a better then average galaxy to look for super nova?

Thanks!
 
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  • #2
Playing Devil's Advocate: is this galaxy red shifted or blue shifted? Are the colors the result of some sort of post exposure processing - color enhancement?

Those are questions I would ask... and your answer is...?

BTW: interesting idea.
 
  • #3
Most galaxies are in general red-shifted because of the expansion of our Universe, right? So odds are it is red-shifted. Wiki says it has a redshift of 0.004657[2] so that means it is red-shifted I think.

https://en.wikipedia.org/wiki/NGC_1398

Is it blue or just processing, good question. I guess I need a power spectrograph of the galaxy to compare to many others. A google image search NGC-1398 shows some not so blue images.

upload_2017-8-5_20-29-52.png


I wonder if there are astronomy databases available to students?

Google seems to think yes, https://www.google.com/search?safe=...k1j33i22i29i30k1j33i21k1j33i160k1.iboIektoTe8
 
  • #4
Why do you think the velocity of a galaxy relative to the Milky Way would make it more or less likely to be a good source of novae? I cannot fathom your logic in this.
 
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  • #5
phinds said:
Why do you think the velocity of a galaxy relative to the Milky Way would make it more or less likely to be a good source of novae? I cannot fathom your logic in this.

If it turns out to be in fact a very blueish galaxy my thoughts are it is then a place of many young hot short lived stars that go boom!
 
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  • #6
Spinnor said:
If it turns out to be in fact a very blueish galaxy my thoughts are it is then a place of young hot short lived stars.
Ah. I was looking at it from the point of view that a galaxy that is almost purely blue shifted could only be so by virtue of it being in the state of having a proper motion towards the Earth and this would have nothing to do with whether or not it is likely to form novae.
 
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  • #7
Spinnor said:
Would this be a better then average galaxy to look for super nova?

I'm not sure about NGC 1398, but it seems void galaxies tend to be bluer as detailed in this paper:

We look at the ur colours as an indication of star formation activity and the inverse concentration index as an indication of galaxy type. We find that void galaxies are statistically bluer than galaxies found in higher density environments with the same magnitude distribution.​

jim mcnamara said:
Playing Devil's Advocate: is this galaxy red shifted or blue shifted? Are the colors the result of some sort of post exposure processing - color enhancement?
Here's some info on the photo: http://skycenter.arizona.edu/gallery/Galaxies/NGC1398
 
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  • #8
From the above link, "Exposure LRGB = 8:4:4:4 Hours", does such an exposure accurately reproduce an image of the galaxy, accurately in the sense that if we were near enough to see the galaxy NGC 1398 with the unaided eye the picture of NGC 1398 above would look like what we saw with our unaided eye?

Thanks!
 
  • #9
The star formation rate (and thus supernova rate) in NGC1398 is quite low: 0.11 Msun/year, or about 7% of what it is in the Milky Way. One photograph that looks blueish is not enough to tell
 
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  • #10
Vanadium 50 said:
The star formation rate (and thus supernova rate) in NGC1398 is quite low: 0.11 Msun/year, or about 7% of what it is in the Milky Way. One photograph that looks blueish is not enough to tell

If star formation rate were low but the proportion of large stars formed was greater we might still get a greater rate of super nova events then for an average galaxy?
 
  • #11
Spinnor said:
From the above link, "Exposure LRGB = 8:4:4:4 Hours", does such an exposure accurately reproduce an image of the galaxy, accurately in the sense that if we were near enough to see the galaxy NGC 1398 with the unaided eye the picture of NGC 1398 above would look like what we saw with our unaided eye?

No to the unaided eye the galaxy would be a grey blob since it is not bright enough to trigger the color receptors in the eye. If you are close enough you might tease out some structure in the blob but that is about it until you get close enough to see individual stars. The reason is that surface luminosity is not affected by distance. If you want to do the comparison yourself go out and look at the Milky way and compare what you see it with the best images of the Milky way (e.g. https://apod.nasa.gov/apod/ap170203.html)
 
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  • #12
Spinnor said:
From the above link, "Exposure LRGB = 8:4:4:4 Hours", does such an exposure accurately reproduce an image of the galaxy, accurately in the sense that if we were near enough to see the galaxy NGC 1398 with the unaided eye the picture of NGC 1398 above would look like what we saw with our unaided eye?

Not really. Even up close the galaxy would be nothing but a "fuzzy blob" of grey, much like how the milky way itself is a greyish streak across the sky and Andromeda is a greyish fuzzy blob, even in a telescope.

More importantly, astronomical images are almost always processed in such a manner as to produce a visually pleasing picture, regardless of what the original "raw" exposures first look like. Many, especially those of nebulas, are entirely wrong in their colors. The "hubble pallet" used to make images from narrowband exposures uses blue to represent the oxygen-III emissions (which are in the blue-green area of the spectrum), green to represent the hydrogen-alpha light (which is actually very, very red), and red to represent sulfur-II emissions (which are slightly more red than the hydrogen-alpha).
 
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1. What is the significance of the "very" blue color in this galaxy?

The "very" blue color in this galaxy indicates that it has a high rate of star formation. The blue color is caused by young, hot stars that emit a lot of blue light.

2. How does the color of a galaxy affect the likelihood of a super nova occurring?

The color of a galaxy does not directly affect the likelihood of a super nova occurring. However, as mentioned before, a galaxy with a high rate of star formation (indicated by a blue color) may have a higher chance of producing super novae due to the presence of young, massive stars.

3. How can we determine if a galaxy is a good place for a super nova to occur?

There are several factors that can determine if a galaxy is a good place for a super nova to occur. These include the presence of young, massive stars, the amount of gas and dust available for star formation, and the overall structure and dynamics of the galaxy. Scientists also use computer simulations and observations of similar galaxies to make predictions about the likelihood of super novae occurring.

4. What role do super novae play in the evolution of galaxies?

Super novae play a crucial role in the evolution of galaxies. They release large amounts of energy and matter into the surrounding environment, which can trigger the formation of new stars and contribute to the chemical enrichment of the galaxy. Super novae also help shape the structure and dynamics of galaxies through their explosive nature.

5. Can we predict when and where a super nova will occur in a galaxy?

While we can make predictions based on certain factors, it is not currently possible to accurately predict when and where a super nova will occur in a galaxy. These events are highly unpredictable and can happen suddenly. However, with advancing technology and further research, scientists may one day be able to make more accurate predictions about super novae in galaxies.

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