... Leda catalogue (cid=1). t=# update galaxies set ra=foo.ra,dec=foo.dec from (select l.al2000 as ra, l.de2000 as dec, g.id from galaxies g, map m, leda.m000 l where g.id = m.gid and m.pid=2 and m.cid=1 and m.cidid = l.pgc ) as foo where foo.id = galaxies.id ...
... m, sn.sn as s where q3c_join(m.al2000*15,m.de2000,s.ra,s.dec,2*(10^(m.logd25-1))/60 ... as s where q3c_join(m.al2000*15,m.de2000,s.ra,s.dec,2*(10^(m.logd25-1))/60.) ) as aa ...
... Credit and Copyright: P. Berlind & P. Challis ( CfA ), 1.2-m Telescope , Whipple Obs . Explanation : What caused the bubbles and arcs in NGC 2359? ...
... Здесь F – сила притяжения , m 1 и m2 – массы двух тел , R – расстояние между ними , G – так называемая гравитационная ... сравнить движение спутника с массой m 1 вокруг тела с массой M 1 и движение спутника с массой m2 вокруг тела с массой М 2 ...
... 2 J.M. Braun et al.: ... 609 \Delta M V =[mag] +0:303 \Delta (M V =[mag]) 2 \Gamma0:036 \Delta (M V =[mag]) 3 ... 8) For star populations one would expect all stars with M2 [18:3; 125] M fi to have ...
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Ссылки http://www.sai.msu.su/groups/cluster/efremov/lmc4/jolh77.ps -- 2727.0 Кб -- 25.07.2002 Похожие документы
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