From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl

Cover From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl
From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl
George Henry Lepper
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Their distribution, so different from that of all other ob- jects, may be considered to show that they have no unity with the rest; but there are other bodies, the stars of Type M for in- stance, which remain indifferent to galactic influence. Indeed, the mere fact that spiral nebulae shun the galaxy may indicate that they are influenced by it. The alternative view is that, lying altogether outside our system, those that happen to be in low galactic latitudes are blotted out by great tracts of ...absorbing mat- ter similar to those which form the dark spaces of the Milky Way.
If the spiral nebulae are within the stellar system, we have no notion what their nature may be. That hypothesis leads to a full stop. It is true that according to one theory the solar system was evolved from a spiral nebula, but the term is here used only by a remote analogy with such objects as those depicted in the Plate. The spirals to which we are referring are, at any rate, too vast to give birth to a solar system, nor could they arise from the disruptive approach of two stars; we must at least credit them as capable of generating a star cluster.


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