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    71. Why Spectral Energy Distributions?
    ... binaries have not been systematically analyzed because the extreme variability of XRBs require simultaneous observations across ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/WhySEDs.html -- 4.0 Кб -- 01.10.2012
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    72. SAO Summer Intern Program Projects, 2002
    ... Ultraviolet Mg II emission is found that signifies a stellar chromosphere -- and ... of these chromospheres can be detected in ultraviolet spectra of the same or similar ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects02.html -- 33.8 Кб -- 01.10.2012
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    73. http://hea-www.harvard.edu/~kim/pap/Blank_2002.pdf
    ... extreme X-ray over optical flux ratio of blanks is not compatible with the main ... Extremely Variable AGNs None of the sources seems to be extremely variable within ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/Blank_2002.pdf -- 679.1 Кб -- 06.12.2010
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    74. http://hea-www.harvard.edu/~elvis/Elvis_AGN_quasar_GCT_CFP.pdf
    ... Quasar central engines also probe extreme conditions of gravity, that could lead us ... Detailed follow-up with optical, ultraviolet and X-ray spectra and light curves can ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/Elvis_AGN_quasar_GCT_CFP.pdf -- 591.9 Кб -- 13.04.2011
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    75. http://hea-www.harvard.edu/QEDT/Papers/phl5200.ps
    ... absorption is common in the optical and ultraviolet spectra of quasars (Ulrich, 1988 ... in velocity width, the BALQSOs may be extreme examples of other associated absorbers ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/phl5200.ps -- 157.4 Кб -- 03.10.1995
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    76. http://hea-www.harvard.edu/~pgreen/PrenHall/earthmoon.txt
    ... hours long. $d) The days and seasons have the same lengths as ours, but the seasons would have more extreme temperature changes ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/PrenHall/earthmoon.txt -- 10.9 Кб -- 10.12.2000
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    77. http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf
    ... The richest and most extreme absorption lines are found in quasars with broad absorption lines (BALs). ... of optically selected QSOs have rest-frame ultraviolet spectra showing these BALsхdeep absorption troughs displaced blueward ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf -- 161.6 Кб -- 14.09.2005
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    78. http://hea-www.harvard.edu/QEDT/Papers/color-color.ps
    ... These outliers are of extreme importance for models since their colors require extreme sets of parameters to explain them. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/color-color.ps -- 787.9 Кб -- 04.04.1995
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    79. http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.ps
    ... The richest and most extreme absorption lines are found in quasars with broad absorp­ tion lines (BALs). ... 10%х15% of optically selected QSOs have rest­frame ultraviolet spectra showing these BALsхdeep absorption troughs displaced ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.ps -- 694.8 Кб -- 14.09.2005
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    80. http://hea-www.harvard.edu/~saku/SDVbiblio2013.pdf
    ... 2008 Ultraviolet Observations of the X-ray Photoionized Wind of Cygnus X-1 during X ... 1997 Hopkins Ultraviolet Telescop e Observations of Her X-1 (B. Boroson, W.P. Blair ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~saku/SDVbiblio2013.pdf -- 95.4 Кб -- 09.12.2013
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