 ... even large and bright ones, offer much greater difficulty in this respect. The cause of this difference must, of course, be conjectural, but, I believe, it is not possible for any one to review seriatim the nebulous contents of the heavens without...  The Intellectual Observer - Page 3471865Full view - About this book
 | 1845 - 774 pages
...its reality as » physical character. Possibly the limits of the conditions of dynamical stability on a spherical cluster, may be compatible with less numerous...comparatively larger individual constituents than in an eliptic one. Be that as it may, though there is no doubt a great number of eliptic nebula; in which... | |
 | William Laxton - 1845 - 564 pages
...nebulous contents of the heavens without being satisfied of its reality as a physical character. Passibly the limits of .the conditions of dynamical stability...larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulae in which stars have... | |
 | 1845 - 880 pages
...nebuloc deviating but little from the spherical from; while, on the other hand, very elliptic nebulre, even large and bright ones, offer much greater difficulty...larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulas in which stars have... | |
 | 1845 - 608 pages
...character. Possibly the limits of the conditions of dynamical stability in я spherical cluster may Ьн compatible with less numerous and comparatively larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulœ in which stars have... | |
 | British Association for the Advancement of Science - 1846 - 520 pages
...which deserves especial remark, and which, now that my own observation has extended to the nebulae of both hemispheres, I feel able to announce with...larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulae in which stars have... | |
 | John M. Lynch - 2000 - 404 pages
...character of easy resolvability into separate and distinct stars is almost entirely confined to nebula; deviating but little from the spherical form ; while,...larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulae in which stars have... | |
 | 1845 - 452 pages
...nebulas deviating but little from the spherical from ; while, on the other hand, very elliptic nebulas, even large and bright ones, offer much greater difficulty...larger individual constituents than in an elliptic one. Be that as it may, though there is no doubt a great number of elliptic nebulas in which stars have... | |
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