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    1. http://www.naic.edu/aisr/bibproj/cache_aeron/DJan.html
    ... Cawley, L. J., J. A. Nousek, G. P. Garmire, D. N. Burrows, D. Janches, and D. H. Lumb, CCD Spectroscopy of the Diffuse X-ray Background, in EUV, X-ray and Gamma-ray instrumentation for Astronomy VI , vol. 2518, edited by O. H. W. Siegmund and J. V ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/aisr/bibproj/cache_aeron/DJan.html -- 11.9 Кб -- 04.05.2007
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    2. http://www.naic.edu/~astro/frontiers/talks/SS_JE_ISM.pdf
    ... Wind? Does the halo have cooler inclusions/phases? superbubbles, winds "Hot Phase" sup What produces the soft X-ray background? ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/frontiers/talks/SS_JE_ISM.pdf -- 963.8 Кб -- 17.09.2007
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    3. http://www.naic.edu/~astro/chicago2/talks/Harrison-HighEnergy-Radio_Connection.pdf
    ... w/ X-ray) observations over wide flux range Focusing in the Hard X-ray Band optics NuSTAR Integral Focal point NuSTAR Pinhole camera High background, large detector, low resolution Low background, compact detector, high resolution Focusing telescope ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/chicago2/talks/Harrison-HighEnergy-Radio_Connection.pdf -- 795.4 Кб -- 21.08.2006
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    4. Diego Janches Information
    ... Educational Background . ... Thesis: Fast Variation of Hard X-ray Emitted in Solar Flares. ... Thesis: Temperature Dependence of the X-Ray Transmission of Optical/UV AXAF Filters. ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/aisr/sas/who/diego.html -- 5.0 Кб -- 08.08.2003
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    5. http://www.naic.edu/~tghosh/higzw/v3.ps
    ... X-ray emission is an ubiquitous property of quasars, and indeed, according to models ... X-rays tend to make the gas too hot to form molecules, and the necessary condition ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/higzw/v3.ps -- 206.2 Кб -- 04.02.2003
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    6. http://www.naic.edu/~tghosh/higzw/v33.ps
    ... X-rays tend to make the gas too hot to form molecules, and the necessary condition ... maser sources, observed in X-rays, show large absorption in soft X-rays (e.g. Wilkes ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/higzw/v33.ps -- 122.7 Кб -- 04.02.2003
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    7. http://www.naic.edu/~tghosh/higzw/feb03-v2.ps
    ... large column density of optically obscuring, X-ray absorbing gas (e.g. Braatz et al ... or a cloudlet within the disk) and the background source, and D is the distance of ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/higzw/feb03-v2.ps -- 107.0 Кб -- 03.02.2003
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    8. http://www.naic.edu/~astro/chicago2/talks/Furlanetto-Cosmology_and_Future_Radio_Telescopes.pdf
    ... 5 km core Before Reionization Pop II Stars SF (2006) The Heating Era X-rays seed fluctuations in TS (and hence Tb) Discrete (biased) sources and 1/r2 flux Soft X-rays have shorter mean free paths Rapid structure formation Also imprints features on power ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/chicago2/talks/Furlanetto-Cosmology_and_Future_Radio_Telescopes.pdf -- 1297.1 Кб -- 21.08.2006
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    9. http://www.naic.edu/~tghosh/a2234/references/srt_report_all_v2.ps
    ... G. 1997, MNRAS 291, 261 5.1.2 Continuum observations 5.1.2.1 Radio Emission from Galactic X-ray Binaries Scienti c Background Relativistic jets, collimated bipolar out ows of matter travelling at a signi cant fraction of the speed of light, appears to be ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/a2234/references/srt_report_all_v2.ps -- 693.0 Кб -- 24.04.2007
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    10. http://www.naic.edu/~tghosh/app06/TG_science.pdf
    ... Earlier generation X-ray satellites (EXOSAT and the Einstein Observatory) had established that X-ray surface brightness distributions in many X-ray bright clusters are centrally peaked, with temperature profiles that decrease (typically by an order of ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/app06/TG_science.pdf -- 70.5 Кб -- 22.11.2006
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