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http://star.arm.ac.uk/~ambn/acl_paper_II.ps.
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1. http://star.arm.ac.uk/~ambn/abstract173.html
In this new series we present observations and modelling of spectral lines formed in main sequence star chromospheres (from G0 to M8). in this paper, we discuss the Hydrogen line formations in very active dMe stellar chromospheres. ... Our final model atmosphere is described in the next paper in this series. ... We found that observations are best reproduced by a chromospheric structure including a constant temperature gradient (in a log(M) scale) in the chromosphere and transition region. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract173.html -- 3.5 Кб -- 31.05.1996
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2. http://star.arm.ac.uk/ext_no.html
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Ссылки http://star.arm.ac.uk/ext_no.html -- 1.3 Кб -- 24.07.2012
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3. Notables in the transition from Fortran 77 to Fortran 90
... The old source code form, which is based on the punched card, and now called fixed form and the new free form. These two forms may not be mixed independently but must be separated at the compilation; an old program, (one or several program units in the form of a main program, subroutines or functions), which is compiled in free form, has the possibility to give a different result compared with earlier when it was compiled with fixed form, compilation errors are possible. ... Comments. ...
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Ссылки http://star.arm.ac.uk/f77to90/c1.html -- 4.1 Кб -- 17.04.1996
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