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1. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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2. Лампочка Luck & Light 5W 3000K Е27 B5W-W Справочник по русскому языку 12296407
... title='Лампочка Luck & Light 5W 3000K Е27 B5W-W' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . Справочник содержит полный курс русского языка для средней школы. В нем в наглядной форме - в таблицах, схемах, памятках - представлены основные разделы русского языка: фонетика, графика и орфоэпия; морфемика (состав слова и словообразование); лексика и фразеология; морфология и орфография; синтаксис и пунктуация. ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku8111.html -- 26.2 Кб -- 14.02.2016
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3. Pulsar Group PmWiki/Forms
... PmWiki .Forms$:Audience} . ... An optional name="FormName" argument can be used to name the form. ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/pulsar/index.html?n=PmWiki.Forms -- 20.7 Кб -- 01.03.2014
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4. OptInt PmWiki : Forms
OptInt PmWiki . ... Forms . ... This page explains how you can embed input forms into wiki pages. ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/Forms -- 29.2 Кб -- 28.02.2014
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5. http://xray.sai.msu.ru/~ivan/gmt/man/sample1d.html
sample1d - Resampling of 1-D data sets sample1d infile [ -Fl|a|c ] [ -H [ nrec ] ] [ -I xinc ] [ -M [ flag ] ] [ -N knotfile ] [ -S xstart ] [ -T x - col ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] sample1d reads a multi-column ASCII [or binary] data set from file [or standard input] and resamples the timeseries/profile at locations where the user needs the values. ... Default is the separation between the first and second abcissa point in the infile ] -M Multiple segment file. ... Default is '>']. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/sample1d.html -- 4.8 Кб -- 19.03.1999
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6. Database of Optical Constants -- Misc: computer codes
The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/JPDOC/0-codes.html -- 4.9 Кб -- 19.11.2010
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7. long
... APPLY/DISPERSION in out [y] [coef] . Apply the dispersion relation to a 1D spectrum and generates a table . BATCH/LONG . ... CALIBRA/FLUX in out [resp] . Correct an image for the instrumental response function . ... Wavelength calibration of 1D and long-slit spectra . ... LINADD/LONG in w,bin [y] [mtd] [mode] [line] . ... PLOT/CALIBRATE [mode] . ... Plots a 1D spectrum in table format, as supplied by APPLY/DISPERSION . ... RESPONSE/LONG [plot] [fit] [deg] [smo] [table] [image] [visu] . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node150.html -- 8.3 Кб -- 23.02.1996
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8. http://www.stsci.edu/instrument-news/handbooks/nicmos/c14_calplan.doc6.html
... The absolute flux calibration of NICMOS will be calculated from observations of standard stars with known flux distributions F( ). ... In order to expand the set of IR standard stars in the appropriate flux range for NICMOS, M. Rieke, R. Thompson, and collaborators at the University of Arizona are making photometric observations of solar-analog stars, which will be used to normalize the solar spectrum to the observed IR magnitudes. ... Relative flux references accurate to 1.5% for standard...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/nicmos/c14_calplan.doc6.html -- 10.7 Кб -- 07.08.1997
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9. http://www.asc.rssi.ru/RadioAstron/documents/memo/ts_eng.pdf
... Tracking stations will be selected in accordance with the schedule issued daily by the General Operative Control Group (GOCG) in Lavochkin Association with the gaps in operations during spacecraft contact with the control stations (CS). ... Communication frequencies (carrier): high data rate information transmission downlink from the SRT ­ 15.000 GHz; uplink synchronization ­ 7.2075 GHz; downlink synchronization ­ 8.400 GHz. ...
[ Текст ]  Ссылки http://www.asc.rssi.ru/RadioAstron/documents/memo/ts_eng.pdf -- 112.7 Кб -- 19.07.2005
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10. Procedure
... Colour transformations are supplied only for the three visual bandpass filter (U, B, V). ... compute the colour term (mag1-mag2) in the instrumental system . select the applicable colour transformation . ... the correct branch of the colour transformation is selected: . match the value of the optional parameter branch (if not set the default value 0 is used) to the value in the column BRANCH of the CCF COLOURMAG extension. the correct interval of the colour transformation is selected: . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node560.html -- 13.0 Кб -- 20.09.2011
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11. http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf
The SCUBA Local Universe Galaxy Survey Dust along the Hubble sequence Catherine Vlahakis University of Bonn Collaborators: Steve Eales (Cardiff University) Loretta Dunne (University of Nottingham) Overview What is SLUGS? Results from the survey Recent work using SLUGS results ­ the FIR-radio relation Introduction: SLUGS SLUGS ­ a submm survey of galaxies in the local Universe ­ at 850m and 450m Survey of ~200 nearby galaxies: 104 60m-selected ("IRS") (Dunne et al. ...
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