'•»

212
* (©. 182.) ©truve, Etudes d'Astr. stcllaire p. 41.
M (©. 182.) Äoemoä $b. I. ©. 156 ttitb 415 «Mnm. 79.
M (©. 183.) »Stars slanding on a clear black ground (@ap--
reif e p. 391). This remarkable bell (the milky way, when
cxamincd Ihrougb powcrful telescopes) is found (wonderful to
rekle!) to consist entirely of stars scattered by mUlions, like
glittering dust, ou the black yround of ihc general heavens.«
(Outlines p. 182, 537 unb 539.)
" (©. 183.) »Globular Clusters, except in one rcgion of
small extent (belween 16 h 45' and 19* in RA.), and nebulae of
regulär elliptic forms are comparatively rare in the Milky Way, and
are found congregated in the grealest abundance in a part of the
heavens the most remote possiblc from that circle.« Outlines
p. 614. ©djon £u»gen$ tvar feit 1656 auf ben Mangel alleä 9te
belö tuib aller 9tebelflecfe in ber 9)?ild)ftraße aufmerffam. 3tt ber=
felben ©teile, in weiter er bie erfie Grntbecfung unb SIbbilbung
beä großen 9?ebelflecfe$ in bem ©ürtel beö Orion bureb einen 28:
füßigen Oiefractor (1656) errcaljnr, fagt er (wie icb febon oben im
2ten 93anbe be$ Äoömoä ©. 514 bemerft): viam lacteam perspicillis
inspeciam nullas habere nebulas; bie 9)iild)ftraße fei wie alle$,
wa$ man für 'Dtebelfterne t>alte, ein großer ©ternbaufen. Sie ©teile
i|i abgebrutft in Hugenii Opera varia 1724 p. 593.
88
(©. 183.) Gap reife 5 105, 107 unb 328. lieber ben
Nebelring 9?o. 3686 f. p. 114.
87
(@. 184.) »Intervals absolulely dark and completely void
of any star of the smallcst lelescopic magnitude.« Outlines
p. 536.
88 (©. 184.) »No region of the heavens is fuller ofobjeets,
beautiful and remarkable in themselves, and rendered still
more so by their mode of associalion and by the peculiar features
assumed by the Milky Way, which are wilhout a parallel
in any other part of its course.« ((Jap reife p. 386.) 25iefer fo
lebenbige 2lu$fprud) »on ©ir 3">b» £erfcbel fiimmt ganj mit ben