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

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Discussion Overview

The discussion revolves around the galaxy NGC 1398 and its potential as a site for supernova occurrences. Participants explore the implications of its color, redshift, and star formation rate, while questioning the validity of photographic representations of the galaxy.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants inquire whether NGC 1398 is a suitable galaxy for observing supernovae, considering its color and characteristics.
  • Questions are raised about the galaxy's redshift or blueshift and whether the observed colors are due to processing techniques.
  • One participant notes that most galaxies are redshifted due to the universe's expansion, suggesting NGC 1398 is likely redshifted based on its reported value.
  • Concerns are expressed regarding the logic of correlating a galaxy's velocity relative to the Milky Way with its potential for supernova events.
  • Another participant mentions that if NGC 1398 is indeed very blue, it could indicate a presence of young, hot stars that are more likely to go supernova.
  • Some participants discuss the star formation rate in NGC 1398, noting it is relatively low compared to the Milky Way, which may affect supernova rates.
  • There is a discussion about the accuracy of photographic representations of the galaxy, with some asserting that images may not reflect what would be seen with the unaided eye.
  • Participants highlight that astronomical images are often processed for visual appeal, which may misrepresent the actual colors and features of celestial objects.

Areas of Agreement / Disagreement

Participants express differing views on the implications of NGC 1398's color and star formation rate for supernova potential. There is no consensus on whether the galaxy is a good candidate for supernova observation, and multiple competing viewpoints remain regarding the interpretation of its characteristics.

Contextual Notes

Limitations include uncertainties about the galaxy's redshift, the effects of image processing on color perception, and the relationship between star formation rates and supernova occurrences.

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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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.
 
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
 
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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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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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.
 
Last edited:
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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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!
 
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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