... The rest may modify the flags register, but this shouldn't matter since gcc should detect it. xchg %bx, %bx is a safe choice for a delay instruction. ...
... assembler or C code into the program or use the system calls mentioned above, it is probably easiest to write a simple C source file with functions for the I/O port accesses or delays that you need, and compile and link it in with the rest of your program ...
... 2 Ring: 216.9 / 27.6 mas 1.2 1.0 Visibility (K-band) 0.8 0.6 0.4 0.2 0.0 2 Ring: 227 ... The thickness of each ring was assumed to be 20% of the ring diameter. ... The thickness of each ring was assumed to be 20 per cent of the ring diameter. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009arXiv0904.1822M.pdf -- 553.9 Кб -- 18.05.2009 Похожие документы
... IRS region S140 is an HII region at the southeast edge of the L1204 dark cloud, located at a distance of 900 pc (Crampton & Fisher 1974), which is part of a cloud complex located at the edge of a prominent infrared emission ring, known as the Cepheus ring ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_381_905W.pdf -- 418.9 Кб -- 03.08.2004 Похожие документы
... 2 Mult icolo ur photome t ry of t he s low nova V2659 Cygni and it s night ly monito ring us ing t he s ma ll te le sc ope s Chochol , D.1, Shugarov, S. 1,2, Krushevska, V.3, Volkov, I.2 1 Astronomical Institute of the Slo vak Academ y of Sciences, Tatr ...
... 0.99109 0.99111 0.99114 0.99116 0.99122 0.99124 0.99126 0.99131 0.99130 0.99134 0.99138 0.99141 0.99144 Ж (deg) (4) 2.7 Ж 1.8 87.4 Ж 0.4 28.8 Ж 0.5 197.3 Ж 0.3 24.8 Ж 0.4 148.6 Ж 1.1 207.5 Ж 0.5 100.0 Ж 0.4 270.9 Ж 0.5 64.1 Ж 0.5 163.1 Ж 0.4 Unres.b Unres ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/205349_web.pdf -- 136.4 Кб -- 05.05.2009 Похожие документы
... The rest wavelength of each DIB was determined in a high quality composite spectrum of the star HD 23180 using the interstellar NaI (D_1 and D_2) lines to establish the radial velocity of the single intervening cloud. ...
... They fitted the interferometric visibilities with simple ring models and found typical inner ring radii ranging from about 0.1 AU for low-luminosity T Tauri stars up to about 10 AU for luminous Herbig Ae/Be stars. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2003/2003A&A_412_735P.pdf -- 972.9 Кб -- 01.02.2005 Похожие документы
... The rest of the paper is divided as follows. ... In the case of KDG 52, the HI is distributed in a clumpy, incomplete ring. ... 4459 and KDG 52, whereas for the rest of the sample galaxies the optical inclination ...
... the subsequent data reduction, we have to rely on a particular model for the cloud ... velocities relative to the local standard of rest are shown on the right, and their ...