... Although the major planets get the most press, a swarm of rocks, comets, and asteroids also exist. ... The light blue lines indicate the orbits of planets . ... Comets appear as dark blue squares, while dark blue points are Jupiter Trojans , asteroids that orbit just ahead of, or just behind Jupiter. Note that most asteroids of the inner Solar System orbit between Mars and Jupiter in the main asteroid belt . ... Publications with keywords: Solar System - asteroid . ... Asteroid and Galaxy . ...

. F IGURE . 3. Plots of V S against cos for the thick disk and the old halo samples. In this graph a constant V rot appears as a straight line. Higher-weight points are plotted with larger symbols. discussion in the text | previous figure | next figure .

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Forecast . Short-term . Map . Long term . N.V. Pushkov . 09/04/2016 23:40 MSK . webmaster@izmiran.ru . Athens . Current Statistics . Chilton . Current Plots . El Arenosillo . Juliusruh . Moscow . Pruhonice . Rome . (C) 2007, IZMIRAN

. If you prefer web-pages with frames, click here. > with(plots):with(linalg): . > A:=matrix(2,2): . > A[1,1]:=1+exp(2*kappa1*x+2*kappa1^3*t+2*theta1)/(2*kappa1): . > A[2,2]:=1+exp(2*kappa2*x+2*kappa2^3*t+2*theta2)/(2*kappa2): . > A[1,2]:=exp((kappa1+kappa2)*x+(kappa1^3+kappa2^3)*t+theta1+theta2)/(kappa1+kappa2): . > A[2,1]:=A[1,2]: . > print(A); . > u:=simplify(-2*diff(log(det(A)),x,x)); . > simplify(diff(u,t)-1/4*diff(u,x,x,x)+3/2*diff(u,x)*u); . 0 . >

Center at RA 02 21 5.48300 DEC 35 56 13.7800 0218+357 IPOL 15359.490 MHZ 0218UN2CM.ICLN 1.1 PLot file version 1 created 03­NOV­1994 19:25:16 Peak flux = 1.3082E­01 JY/BEAM Levs = 1.5000E­03 * ( ­2.00, ­1.00, 1.000, 2.000, 4.000, 8.000, 16.00, 32.00, 64.00, 128.0, 256.0, 512.0) MilliARC SEC MilliARC SEC 314 313 312 311 310 309 308 307 306 131 130 129 128 127 126 125 124

set timefmt '%Y-%m-%d %H:%M:%S' set xdata time set title 'MASTER-NET CGRaBS J0211+1051 Unfiltred observation' set ylabel 'Magnitude' set xlabel 'Time' set term gif set output 'lc.gif' set yrange [] reverse unset key set format x '%Y' set grid plot 'lc.cat' u 1:4 w p notitle , 'lc.cat' u 1:4:5 w errorbar

ENEIDE = E sperimento di N avigazione per E vento I taliano D imostrativo di E GNOS. His ego nec metas rerum nec tempora pono' (For these men I plot no course, nor do I set limits for their work) (Aenead, I, 278). ...

Neutron Monitors ] [ Solar Neutrons ] [ Muon Telescopes ] [ Base Potchefstroom University ] [ Magnetometers ] [ GPS systems ] [ Ionosphere ] [ Related Data ] [ Space Weather ] . ... All Cosmic Ray Stations + InterPlanetary Data: WorldNet . Alma-AtaB (Mt.Tien Shan) DataBase of Kazakhstan Spectrograph Alma-AtaB (Mt.Tien Shan) new . ... Nagoya Muon Telescope and DATA or mail . ... Belgrade Muon Telescopes and DATA or ">mail . ... Real-Time database for Cosmic Ray Anisotropy (DB10) . ...

... Bad Astronomy . ... Movies . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Space Cowboys . ... He used a lot of real NASA simulators and technology, and filmed a lot of the movie on location at Johnson Space Center and Kennedy Space Center. ... Since this was a first-run movie, I'll put my Bad Astronomy review on a separate page. Be warned: if you haven't seen the movie, the review will spoil the plot. CLICK HERE TO GO TO MY REVIEW OF ``SPACE COWBOYS''. ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

Magnetic Stars, 2011, pp. ... Key words: instrumentation: polarimetry ­ magnetic fields ­ stars: individual (WD1658­441) ­ stars: magnetic fields ­ stars: white dwarfs 1 Intro duction Low­resolution spectropolarimeters are intended mainly for spectropolarimetric studies of faint ob jects. ... Magnetism of white dwarfs. ... 223 Figure 4: Spectrum (upper plot) and circular polarization (lower plot) of the zero polarization standard maximal rotationally modulated longitudinal magnetic field. ...

... It is known from preliminary observations that the period of this binary star is more than 8 hours but less than 12 hours. O. Struve & V. Zebergs (1959, ApJ, 130, 783) measured radial velocities of the two components and get the results presented at the enclosed "sheet of data". ... Plot graph of the velocities of components vs time. 8.2. Find exact orbital period of the components. ... Find exact orbital period, orbital radius and masses of the two components. ...

... Hu ChangSong for his Chinese translation * Ciprian Manea for his Romanian translation * Neil Muller for his suggestions on making bbclone work with register_globals off * Carlos Oliva for his Spanish translation * Vilius Simonaitis for his Lithuanian translation * Chad Schmidt for his numerous corrections * Gregori Arjona for his Catalan translation * Engelbert Gruber for his suggestions on correcting fopenlock() * Josef Pinc for his Czech ...