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    31. GSAOI Magellanic Cloud Planetary Nebulae Science Page
    ... In the infrared, the nebula can be mapped in the 2.122 m 1-0 S(1) and 2.248 m 2-1 S(1) lines of molecular hydrogen, which in most objects seem to be fluorescently excited by UV radiation from the central star. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/pne.shtml -- 8.4 Кб -- 01.10.2012
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    32. Observational Techniques Home Page
    ... Statistics Notes: Part 2 . UV/Optical/IR Astronomy Notes . Spectroscopy notes . Topics will not be covered in precisely this order. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/ObsTech/ -- 5.7 Кб -- 01.10.2012
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    33. http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/doppler.pdf
    ... Blue: 400 nm Red: 700 nm Visible Gamma Rays 10 -12 X-Rays UV Microwaves Radio Waves Infrared UHF FM FM 10 -4 10 -8 1 10 4 Wavelength (metres) · These are all basically the same things: waves of entwined electricity and magnetism flying through space: the ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/doppler.pdf -- 841.5 Кб -- 09.08.2004
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    34. Key formulae
    ... Cooler objects emit most of their radiation in the red or IR, while hotter objects emit in the UV or even in the X-rays.. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/thermodynamics.htm -- 15.5 Кб -- 09.08.2004
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    35. http://www.mso.anu.edu.au/seminars/abstracts/20150512-1100.html
    ... Many of these questions are being addressed by recent projects that combine UV and high-angular resolution with the Hubble Space Telescope, and which I will describe together with the results they have obtained so far. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150512-1100.html -- 4.7 Кб -- 10.04.2016
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    36. http://www.mso.anu.edu.au/~bessell/FTP/Filters/Epotek301-2FL.pdf
    ... The product can resist yellowing over 17 days of continuous UV light exposure. Suitable for LED encapsulation. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Filters/Epotek301-2FL.pdf -- 166.2 Кб -- 07.03.2011
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    37. http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt
    ... The blue colour represents the 164nm Uv band, the green is V and red is Halpha. the pink stars are Be stars, that is, blue stars with strong Halpha emission. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt -- 8.7 Кб -- 27.01.2004
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    38. http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf
    ... far infrared (Hz) (Angstroms) (metres) 0.20 100 10 = 10 ­6 (eV) 6.2 10 1.1 10 0.62 2.48 12.4 ­6 ­2 ­4 Typical near infrared Typical optical Typical UV Soft X-ray Hard X-ray TeV -ray 2.41 10 2.41 10 2.41 10 17 19 26 2 10 5000 1000 12.4 0.124 1.24 10 ­8 ­6 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf -- 117.5 Кб -- 04.08.2009
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    39. http://www.mso.anu.edu.au/pfrancis/roleplay/greenhouse.doc
    ... Unless it is exposed to strong ultra-violet (UV) light, that is. ... the water vapor steamed off the surface of the water, the UV light from the tanning lamps (designed to mimic the healthy rays ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/greenhouse.doc -- 34.5 Кб -- 21.03.2000
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    40. Untitled1
    ... Contributed talk: "UV Diagnostics for the Emission Line Gas in Active Galaxies ... Contributed talk: "UV Diagnostics for Emission line Gas". ... Contributed poster: "UV Emission Line Diagnostics". Dr T Axelrod . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/11_staffAct.html -- 51.3 Кб -- 02.10.2012
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