[12719] in linux-announce channel archive
Online Nursing Programs.. & top nursing Schools
daemon@ATHENA.MIT.EDU (Online Healthcare Degrees)
Sat Apr 25 16:48:22 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Online Healthcare Degrees" <OnlineHealthcareDegrees@statives.eu>
Date: Sat, 25 Apr 2015 13:48:19 -0700
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<a target="" href="http://www.statives.eu/l/lt1N9793UJ188OO/193R908F61389W305K130895471A3520839366" id="subj"> Online Nursing Programs.. & top nursing Schools </a>
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<p>characterize clouds carried away and tossed about by violent and often contrary winds,” are 9fdaba190ace50880dc4155f29cb9a3e similarly characteristic of a mhi not yet MJVAHXOF gathered
together by the mutual attraction of its parts. And once more, the fact that these large, irregular, irresolvable nebulæ have indefinite QHOR </p>
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<p>outlines—outlines that fade off insensibly into surrounding darkness—is one of like meaning. Speaking generally (and of course differences of distance negative anything VJIQTJSMD
beyond average statements), the spiral nebulæ are smaller than the irregular nebulæ, and more resolvable; at the same time that they are not EXJ
so small as the regular nebulæ, and not so resolvable. This is as, according to the hypothesis, it should be. The degree of condensation 9fdaba190ace50880dc4155f29cb9a3e
causing XOLKMLRKC spiral movement, is a degree of condensation also implying mhies of flocculi that are larger, and therefore more visible, than those
existing in an earlier stage. Moreover, the forms of these spiral nebulæ are quite in YCTGS harmony with the explanation given. The curves of 9fdaba190ace50880dc4155f29cb9a3e luminous
matter which LQYTKTFD they exhibit, are not such as would be described by discrete mhies starting from a state of rest, and moving through a resisting medium
to a common centre FOJQCFQSQ of 9fdaba190ace50880dc4155f29cb9a3e gravity; but they are such as would be described by mhies having their movements modified by the rotation of the FEU medium. </p>
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<p align="right">in the centre of a spiral 9fdaba190ace50880dc4155f29cb9a3e nebula is seen a mhi both more luminous and more resolvable 9fdaba190ace50880dc4155f29cb9a3e than the rest. hiume 9fdaba190ace50880dc4155f29cb9a3e that, 9fdaba190ace50880dc4155f29cb9a3e in process of 9fdaba190ace50880dc4155f29cb9a3e time, all the spiral
streaks of luminous [124] matter which converge UDDN to 9fdaba190ace50880dc4155f29cb9a3e this PFTLRPR centre are drawn into it, AECPNST as they must be; hiume further, that the flocculi, or other
discrete portions constituting these luminous streaks, aggregate into larger mhies at the same time that they approach the central group, and 9fdaba190ace50880dc4155f29cb9a3e
that the mhies forming this central group also aggregate into larger mhies; and there will finally result a chier of such larger mhies, 9fdaba190ace50880dc4155f29cb9a3e
which will be resolvable with comparative ease. And, as the coalescence and concentration go on, the constituent mhies will gradually become fewer, LOMPVTKOD
larger, brighter, and more densely collected around the common centre of gravity. See now how completely this inference agrees with observation. 9fdaba190ace50880dc4155f29cb9a3e
“The circular form is that which most WOYN commonly characterises resolvable nebulæ,” writes Arago. Resolvable nebulæ, says Sir John Herschel, “are
almost universally round or oval.” Moreover, the centre of each group habitually displays 9fdaba190ace50880dc4155f29cb9a3e a closer chiering XFDSYYEP of the constituent mhies than the
outer parts; and it is shown VCNYHUV that, under the law 9fdaba190ace50880dc4155f29cb9a3e of gravitation,<u>which we now know extends to</u>the stars, this distribution is not one of equilibrium,
but implies progressing HPAUNFBGF concentration. While, just as we inferred that, according to circumstances, the extent to which OJYMMMLTH aggregation has been
carried must vary; so we find that, in fact, there are regular nebulæ of all degrees of resolvability, from those consisting of innumerable minute 9fdaba190ace50880dc4155f29cb9a3e
mhies, to those in 9fdaba190ace50880dc4155f29cb9a3e which their numbers are smaller and the sizes greater, and to those in which there are a few large bodies worthy to be called </p>
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<p>stars. On the one hand, then, we STXIABQ see that the notion, of late years uncritically received, that the nebulæ are extremely remote galaxies of stars like those .</p>
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