214 



ol Ihc iield ol view). @. in ter (Japreife p. 390 bew Slbld^iiitr: 

 »011 some indications of very remote telescopic branchcs of Ihe 

 Milky Way, or of an independent sidereal System, or Systems, 

 bearing a resemblarice to such braiiches.« 



" (@. 189.) e« pr eife 5 314. 



»• (@. 189.) eir SBtUiam .^erfc^el i\\ ben Philos. Trans- 

 act. tor 1785 p. 21; @ir 3ol)n ^crfd)el, ßapreife § 293. 

 (iBer^l. m<i) ©truoe, Descr. de l'Observaloire de Poul- 

 kova 1845 p. 267-271.) 



"' (@. 189.) )ilthink«, i'avjt ®ir ^C'i)\\ s>ex{d)ei, »it is im- 

 possible to view Ihis splendid zone from a Ceiitauri to the Gross 

 without an impression amounting almost to conviciion, that the 

 milky way is not a mere Stratum, but annutnr; or at Icnst that 

 our System is placed wilhiti one ol" the poorer or almost vacant 

 parls ol its general mass, and that eccentricaliy, so as to be 

 much nearer to the region about Ihe Gross than to that dianie- 

 irically opposite to ii.« (?Oiary ©onieruille on the conne- 

 xion of the physical sciences 18^6 p. 419.) 



'"" (@. 189.) (Jöpreife § 315. 



