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    51. http://www.mso.anu.edu.au/~geoff/HEA/Solns_Q_1-8.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/Solns_Q_1-8.pdf -- 147.7 Кб -- 18.03.2015
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    52. http://www.mso.anu.edu.au/~geoff/HEA/11_Accretion_Disks_II.pdf
    ... This the reason proposed for the UV bumps shown in the spectra of AGN at the left. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/11_Accretion_Disks_II.pdf -- 813.5 Кб -- 12.06.2003
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    53. http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf
    ... 1994 photo-ionized by anisotropic nuclear UV radiation perhaps originating from the ... Theoretical work indicates that UV X-ray radiation from the central engine can heat ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf -- 623.9 Кб -- 31.05.2000
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    54. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Chemin06
    ... In order to get a better uv plane coverage, the hybrid DnC configuration, with ... First, the uv datasets were carefully examined to detect and reject bad points due ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Chemin06 -- 513.6 Кб -- 16.05.2007
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    55. http://www.mso.anu.edu.au/~bessell/bescast.pdf
    ... and in the precision and accuracy of observed colors of stars from the UV to the IR ... determination and fluxes measured further into the UV such as with the WPFC2 filters ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/bescast.pdf -- 412.6 Кб -- 09.04.2006
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    56. http://www.mso.anu.edu.au/~bessell/Beauty.ps
    ... is also the transformation of images made in passbands in the UV, IR or radio into optical colours that enhances our insights ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/Beauty.ps -- 139.3 Кб -- 28.01.2004
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    57. http://www.mso.anu.edu.au/~raquel/Hawaiiposter.pdf
    ... the innermost object are non-thermal: Interstellar cosmic rays, emitted by the magnetically active p rotostar and elements present in the disk (see schematic diagram, ~ 0.1 AU from the central X-rays and UV radiation the decay of radioactive left panel ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~raquel/Hawaiiposter.pdf -- 159.5 Кб -- 06.01.2008
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    58. Untitled1
    ... This emission was expected from the ionization of the diffuse outer HI by the metagalactic UV radiation field. ... stronger than expected, and suggests that the ionization comes from UV photons emitted by the inner disk of the galaxy itself ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/07_research.html -- 73.5 Кб -- 02.10.2012
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    59. Index of /~bessell/FTP/Oldspectrophotometry
    ... F110 is a sdO star with weak He and H lines and much UV flux. ********** l745-46anew.tab, hd26169.tab and ltt4364new.tab are determined by Bessell in Jan 2009 using the Gregg-Heap spectra as standards. **************** 2) bessell2007BJ.pdf is a 2007 PASP ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/ -- 25.4 Кб -- 02.10.2012
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    60. http://www.mso.anu.edu.au/~bessell/FTP/PARTF__12ptnew.doc
    ... These include the Balmer discontinuity and spectral features such as the CaII H and K lines and the CN bands in the UV. ... These use expensive, exotic and fragile materials, such as CaF2 and high refractive index UV- efficient glasses. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/PARTF__12ptnew.doc -- 551.0 Кб -- 08.05.2006
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