Why is Far-UV spectrum unobservable

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SUMMARY

The far-UV spectrum is unobservable primarily due to strong absorption by hydrogen and interstellar dust, which intercepts radiation at these wavelengths. Observations of Active Galactic Nuclei (AGN) are hindered by the obscuration from dust torii surrounding the accretion disk, especially when viewed at certain angles. Additionally, Earth's atmosphere effectively blocks UV light, necessitating the use of space-based telescopes for UV observations. The literature, including "The Physics of AGN at All Scales" from Springer, provides further insights into these phenomena.

PREREQUISITES
  • Understanding of Active Galactic Nuclei (AGN)
  • Knowledge of hydrogen absorption spectra
  • Familiarity with interstellar dust properties
  • Awareness of space-based telescopes and their applications
NEXT STEPS
  • Research the mechanisms of hydrogen absorption in the UV spectrum
  • Study the role of interstellar dust in astronomical observations
  • Explore the design and capabilities of space-based UV telescopes
  • Investigate the impact of Earth's atmosphere on astronomical observations
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Astronomers, astrophysicists, and students studying the properties of light in space, particularly those focusing on the observation of Active Galactic Nuclei and the challenges of UV astronomy.

PianoDentist
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Hi

couldn't find a similar thread so thought i'd make one. I keep seeing around the web that the far-UV spectrum is unobservable (context is looking at the spectra of AGN) but no-one seems to explain why.

I think that its something to do with hydrogen strongly absorbs at these wavelengths so all the dust between us and what we're looking at intercepts all the radiation at these wavelengths.

But I am not sure if this is the case and I am not sure why hydrogen/ or interstellar dust would absorb strongly at these far UV frequencies.

if anybody can explain why the far-uv is unobservable that would be greatly appreciated!
 
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I am inferring this from the literature on AGN I've read but I am by no means confident in what I am saying: I think the optical & UV comes mainly from the accretion disk, which is generally obscured by the dust torii that surround it if it's observed sideways. The jets get in the way for compact objects that are at smaller inclination angles wrt the jet axis. So I think that's why it might by difficult to resolve disk UV emission specifically from other structures like the NLR clouds.

"The physics of AGN at all scales" (Springer) might have the answer to your question.
 
Earths atmosphere is extremely efficient at blocking UV light - which is good because it keeps the sun from sterilizing the surface of the earth. Life on Earth was limited to the oceans until the atmosphere became oxygenated and the ozone layer formed. To observe the universe in the UV spectrum requires space based telescopes. See http://www.britannica.com/EBchecked/topic/613577/ultraviolet-telescope for discussion.
 

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