... m 12/56 For relatively nearby sources: cz D = -----H0 Cygnus A: z = 0.056075 D = 243 ... M * c 2 High Energy Astrophysics: Radio Galaxies 17/56 Therefore, if all the energy ...
... De Propris, R., Stanford, S., Eisenhardt, P., Dickinson, M., (2003) "The K-Selected Butcher-Oemler Efffect", Astrophysics and Space Science, Vol 285, Issue, pp 43-47. ...
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... tGU T tbar y ogenesis telectr oweak tBBN tr -m tr ec t1stther m-dis t1ststar s t1stE ar ths tr now tS un ,tE ar th tm- to tlaststar s tpr otondecay tblackholes theatdeath Time after seconds 5.4 в 10-44 [10-43 , 10-33 ] 10-33 -33 , 10-12 ] [10 10-12 [100 ...
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... m ) are given by: dt 1 ---- = m = -- m a ds 1 dt dt d t dt ... mm (31) High Energy Astrophysics: Synchrotron Radiation I 34/106 The critical ... m e c 2 dt m e c B 2 2 2 ----- sin o (102) (101) High Energy Astrophysics ...
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... M a + MX - M b - M Y ) = M a + M X - M b - M = 2 .4 2 4 7 5 + 0 - ( - 4 .7 3 6 5 5 ... m a ssiv e st a rs ( 8 M su n a n d a b o v e ) , a n d d u r i n g H e - b u r n i ...