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    • 1 | 2 | След.

    1. Astrophysics Group AMI Publications
    ... GRB 090313 and the Origin of Optical Peaks in Gamma-ray Burst Light Curves: Implications for Lorentz Factors and Radio Flares . ... A change in the optical polarization associated with a gamma-ray flare in the blazar 3C279 . Abdo A. A. et al., ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/facilities/ami/ami-publications/ -- 30.8 Кб -- 10.04.2016
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    2. http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI-Fender.pdf
    ... emission from Cygnus X-3 during phases of radio flaring ­ 'extreme' particle acceleration in the jet (via interaction with the ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI-Fender.pdf -- 1336.8 Кб -- 04.10.2011
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    3. An expanding plasmon model for the radio outbursts of Cir X-1
    ... to account for the double-peaked radio flares from Cir X-1, observed at multi ... At 1.4 and 2.3 GHz the flare is broad and does not seem to have double-peaked ... ejection events have been considered to account for the double-peaked flare observed ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/garcia/garcia.html -- 13.7 Кб -- 08.12.2003
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    4. http://www.mrao.cam.ac.uk/yerac/garcia/garcia.ps
    ... to account for the double­peaked radio flares from Cir X­1, observed at multi ... b) At 1.4 and 2.3 GHz the flare is broad and does not seem to have double­peaked ... ejection events have been considered to account for the double­peaked flare observed ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/garcia/garcia.ps -- 204.8 Кб -- 22.02.1995
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    5. http://www.mrao.cam.ac.uk/~guy/microq6.pdf
    ... The great flares of Cygnus X-3 in 1972, which were reported in a whole issue of ... Cyg X-1 does not show the bright radio flares associated with Cyg X-3, for example ... There are flares on Cyg X-1, not as spectacular and very much rarer (I have only ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~guy/microq6.pdf -- 1951.6 Кб -- 19.01.2007
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    6. G111.7-2.1
    ... ADS . Fesen et al. 1988, ApJ, 329, L89. Optical, flocculli, and ``flare". ADS . Jansen et al. 1988, ApJ, 331, 949. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-1996/snrs.G111.7-2.1.html -- 7.9 Кб -- 10.04.2016
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    7. G111.7-2.1
    ... ADS . Fesen et al. 1988, ApJ, 329, L89. Optical, flocculli, and `flare'. ADS . Woan & Duffett-Smith 1990, MNRAS, 243, 87. Structure at 81.5 MHz. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-1998/snrs.G111.7-2.1.html -- 9.3 Кб -- 10.04.2016
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    8. Astrophysics Group Research and Instrumentation
    ... M dwarfs often exhibit significant stellar variability (due to star spots and flares) that render the search for transiting planets challenging. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/research/exoplanets/research/ -- 22.7 Кб -- 10.04.2016
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    9. http://www.mrao.cam.ac.uk/~bn204/almasim08/papers/64_50_presentaion_2008a.pdf
    ... Time Gain: we can track time changes to the same senstivity faster by (64/50)^2 = 1.64 Very fast mm variability is rare (solar flares?) ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/almasim08/papers/64_50_presentaion_2008a.pdf -- 1160.4 Кб -- 02.12.2008
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    10. http://www.mrao.cam.ac.uk/~eic22/Papers/scaife10.pdf
    ... 23 22 59 02 00 46 36 57 19 08 23 24 02 05 60 09 46 39 Association Taurus Taurus Aquila Rift, Cloud B Aquila Rift, Cloud B Aquila Rift, Cloud B Cepheus Flare Cepheus Flare Cloud 157, Cyg OB7 SCUBA Y/N Y Y Y Y N N Y Y N Y Y N Y MAMBO Y/N N Y N N Y Y N N Y Y ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~eic22/Papers/scaife10.pdf -- 1198.0 Кб -- 03.09.2010
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