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1. http://www.mrao.cam.ac.uk/yerac/koester/koester.ps
... We present observations of the [CII] 158 Їm and 12 CO 3 ! 2 line emission of the Rosette Molecular Cloud. ... We use a plane­parallel finite sized PDR model with a wide range of densities and UV field strengths in order to model the observed regions. ... These PDR models succeed to explain the observed line integrated intensities of e.g. the low­ and mid­J 12 CO rotational lines or the [CII] 158 Їm line both in galactic sources (star formations regions) and external galaxies (e.g. Wolfire et al. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/koester/koester.ps -- 168.3 Кб -- 22.02.1995
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2. http://www.mrao.cam.ac.uk/~mh475/5Dec08.html
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~mh475/5Dec08.html -- 1.0 Кб -- 05.12.2008
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3. http://www.mrao.cam.ac.uk/projects/aavp/posters/daSilva_AAVP-Cambridge2010.pdf
... The design employs a differential structure. ... The input is adapted to 100 differential, and the outputs use standard Low Voltage Differential Signaling (LVDS). ... T/H SINGLE T/H Single Input T/H Single Output 1.35 0.15 0.2 T/H DIFFERENTIAL Input T/H Output T/H 0.1 1.3 0.05 volts volts Figure 5: Digital part and digital gate 0 1.25 -0.05 -0.1 1.2 Integrated Test System A test system is integrated on chip to evaluate the transmission to the data acquisition card (fig: 7). ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/aavp/posters/daSilva_AAVP-Cambridge2010.pdf -- 1772.7 Кб -- 06.12.2010
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