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    1. http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf
    ... with VLA radio inset, showing clear feedback between radio jets and cluster gas ... them strong candidates for central feedback to offset excess cluster gas cooling ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf -- 2276.9 Кб -- 26.04.2013
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    2. http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI_Day_Presentation_hogan.pdf
    ... Feedback needed to offset cooling and explain the deficit of cold, molecular gas in cluster cores. ... feedback required to explain the deficit of cold, molecular gas in cluster cores Radio analysis of BCGs complicated by presence ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI_Day_Presentation_hogan.pdf -- 2534.2 Кб -- 04.10.2011
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    3. http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/bartlett.ps
    ... Because we believe that the hot cluster gas is heated by infall during cluster ... tot is the total, virial mass of the cluster, f gas is the hot gas mass fraction of ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/bartlett.ps -- 131.7 Кб -- 25.07.1997
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    4. http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/birkinshaw.ps
    ... a more detailed ex­ amination of the cluster's gas content than the Einstein data ... 1, and are a good match to a model for the cluster gas based on the X­ray image ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/birkinshaw.ps -- 178.6 Кб -- 22.06.1997
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    5. http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/grainge.ps
    ... that, on large scales, the intra­cluster gas is typically very close to being ... insensitive to the low density gas far from the cluster centre (see equation 2), and ... 4.2 Cooling Flows In many clusters the gas density is sufficiently high at the ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/grainge.ps -- 2920.2 Кб -- 27.06.1997
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    6. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect3.pdf
    ... н Blackbody н "Flat" Example: X-ray emission from clusters of galaxies Gas in clusters of galaxies at temperatures of . ... Therefore Bremsstrahlung emission extends into X-rays. Cluster gas also gives rise to the SunyaevнZel'dovich effect . ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect3.pdf -- 420.8 Кб -- 17.10.2003
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    7. http://www.mrao.cam.ac.uk/~krause/krause04.apss.pdf
    ... the X-ray appearance of the shocked cluster gas and compare it to Cygnus A and 3C ... shown that the jets have a considerable impact on the cluster gas (Carilli et al ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~krause/krause04.apss.pdf -- 1531.9 Кб -- 14.02.2005
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    8. http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/molnar.ps
    ... SSC by extrapolating the gas mass and luminosity relation for clusters of galaxies ... distribution of the intra­(super)cluster diffuse gas strongly depend on the dynamics ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/molnar.ps -- 134.4 Кб -- 22.06.1997
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    9. http://www.mrao.cam.ac.uk/~anthony/latex/Myers.ps
    ... The SZE is caused by Compton scattering of low-energy CMB photons o high- temperature ionized gas in cluster atmospheres, and is a direct measurement of the baryon content of the intercluster medium. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Myers.ps -- 22.5 Кб -- 15.06.2000
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    10. http://www.mrao.cam.ac.uk/~krause/krause04.aa.small.pdf
    ... T = 3 в 107 K. The cooling time in the shocked cluster gas is approximately 100 Myr ... cocoon on the left-hand side, and the entrained cluster gas on the right-hand side ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~krause/krause04.aa.small.pdf -- 2082.8 Кб -- 14.02.2005
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