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http://lnfm1.sai.msu.ru/neb/nss/OBS_COLL/ElemSat.txt.

1. http://lnfm1.sai.msu.ru/neb/nss/OBS_COLL/ElemJup.txt
... 5, 20:35 UT For S/2000 J 2 - S/2000 J 11 Epoch of mean anomaly 2001 Apr. ... Mean Pericenter Node , of of mean motion, demi-axe, deg anomaly from node , deg M.P.E.C. satellite anomaly,TT deg /day ua at epoch , deg (relative to the geoecliptic J2000), deg ------------------------------------------------------------------------------------------------------------- 2000 -Y16 S/1999 J 1 2452000.5 0.48920131 0.1570775 0.2061509 143.48974 294.79692 56.96157 282.84304 S/ ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/OBS_COLL/ElemJup.txt -- 11.9 Кб -- 11.12.2003
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2. Stellarium: core/planetsephems/elliptic_to_rectangular.h Source File
Stellarium 0.12.3 . ... FileљStructure . ... core . planetsephems . elliptic_to_rectangular.h . ... 8 љ obtained from above and rearranged it into this piece of software. ... 19 љ copy of this software and associated documentation files (the "Software"), . ... 53 љ elem[0] .. unused (eigther a or n) . ... K=e*cos(Omega+omega) . ... 70 љ void EllipticToRectangularN( double mu, const double elem[6], double dt, . ... 72 љ void EllipticToRectangularA( double mu, const double elem[6], double dt, . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/elliptic__to__rectangular_8h_source.html -- 15.2 Кб -- 28.02.2014
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3. Astronomy Letters, Volume 2
... PAZh: 3-9 ; SvAL: 1-3 ) . COSMOS-428 observations of hard X-rays from galactic center . ... Light curve of Nova Cygni 1975 (V 1500 Cyg) . ... Infrared observations of Nova Cygni 1975. ... Observations of the X-ray source Hercules X-1 on board of the space station SALYUT-4 . ... Observations of intense X-ray bursts from Cyg X-1 . ... Observations of the X-ray source Cir X-1 on board of the space station SALYUT-4 . ... Scorpius X-1 - observations from the SALYUT-4 station in Janyary 1975 . ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/~sergei/pazh/pazh1976_02.html -- 31.6 Кб -- 28.05.2013
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4. http://hea-www.harvard.edu/~srandall/M86/m86.pdf
... We detect three main diffuse components: the Virgo ICM at 2.4 keV, the extended halo of M86 at 1.2 keV, and the cooler central and stripped gas of M86 at 0.8 keV. ... The data are inconsistent with a radial orbit, and imply inner and outer turning radii of ri 300 kpc and ro 8.8 Mpc, indicating that M86 is, at best, only weakly bound to the Virgo cluster. ... Constraints on the Orbit of M86 5 Knowing the orbit of M86 is the key to understanding its interaction with the Virgo cluster. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~srandall/M86/m86.pdf -- 2563.0 Кб -- 07.03.2011
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