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    1. http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Pictor_A.pdf
    ... out a faint (40 - 50 counts above the background), compact X-ray source 323 E of the ... X-ray spectrum Given the low count rate, the background begins to dominate above 2.5 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Pictor_A.pdf -- 324.7 Кб -- 06.05.2001
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    2. http://www.mso.anu.edu.au/~charley/papers/Dopita2011.pdf
    ... More importantly, if there were many fainter quasars producing sufficient UV to reionize the universe at z = 10, then they would overproduce the present-day unresolved soft X-ray background (Dijkstra et al. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/Dopita2011.pdf -- 414.2 Кб -- 19.10.2011
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    3. Pink Black Holes: Technical Details
    ... Pink Black Holes: Technical Details . Background . Colours. ... page is intended for those with a technical background who want more detail than was ... Many are reasonable X-ray sources as detected by ROSAT (Seibert et al. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/pink/tech.html -- 5.3 Кб -- 01.10.2012
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    4. http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf
    ... 5.4 The microwave background The dipole component of the Cosmic Microwave background ... of the microwave background Spectrum of the microwave background as measured by COBE ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf -- 2636.4 Кб -- 04.03.2001
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    5. Paul Francis -- Astronomical Constants
    ... Cosmic Microwave Background Formation. ... shows the formation of the Cosmic Microwave Background (CMB) at a detailed level ... is these undisturbed photons that form the cosmic microwave background we see today ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/simulations/ -- 14.5 Кб -- 09.04.2016
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    6. http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Cygnus_A.pdf
    ... X-ray observations of the powerful radio galaxy Cygnus A with the Chandra X-ray ... X-rays - thermal and synchrotron emissions - and the poor spatial and spectral ... When the X-ray and radio nuclei are aligned, the compact X-ray sources at the SE and ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Cygnus_A.pdf -- 109.1 Кб -- 06.05.2001
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    7. http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf
    ... of the Universe is 2.73 degrees K as seen in the Cosmic Microwave Background ... law), show that the cosmic microwave background radiation continues to follow Planck ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf -- 262.1 Кб -- 02.09.2009
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    8. http://www.mso.anu.edu.au/~kcf/pubs_top20/54.pdf
    ... X-ray Observatory as part of our approved program for the SHBs, observing the 81-arcsec error circle with the Advanced CCD Imaging Spectrometer (ACIS).11 A total of 38.4 ks of go o d data were obtained after excluding intervals of background flaring ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/54.pdf -- 330.7 Кб -- 15.10.2011
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    9. http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf
    ... This is often the case at the bases of jets, so that these regions are often strong X-ray emitters. ... 5 Inverse Compton emission from the microwave background A regime in which inverse Compton emission is important is in the ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf -- 105.7 Кб -- 27.05.2003
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    10. http://www.mso.anu.edu.au/~geoff/HEA/6_Compton_Scattering_II.pdf
    ... spots in Cygnus A. The radio image is shown as a greyscale; the X-ray image is shown as contours overlaid on the radio image ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/6_Compton_Scattering_II.pdf -- 430.6 Кб -- 27.05.2003
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