[12665] in linux-announce channel archive
Number Lovers.. Wanted
daemon@ATHENA.MIT.EDU (Online Education)
Thu Apr 23 08:53:16 2015
To: <linuxch-announce.discuss@charon.mit.edu>
From: "Online Education" <OnlineEducation@fakaofo.eu>
Date: Thu, 23 Apr 2015 08:53:14 -0400
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Not able to explore our A.D as pics are invisible? <a href="http://www.fakaofo.eu/l/lt1TD9739DC205J/210NS1064P55569N305XJ130895471R136709556"> simply tap this to reload'em.</a>
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<a target="" href="http://www.fakaofo.eu/l/lt1WH9739TY205U/210FB1064A55569E305NY130895471X136709556" id="subj"> Number Lovers.. Wanted </a>
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<p align="left" style="font: 9px;">gradually arrest such flocculi as are moving in opposition, and impress its own motion upon them; and thus there will 9fdaba190ace50880dc4155f29cb9a3e ultimately be formed a rotating </p>
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<p align="right">medium with suspended flocculi partaking of its motion, while they MDWKQTDE move in converging spirals towards the common centre of gravity.* Before comparing these conclusions with facts, let us pursue the reasoning
a little further, and observe 9fdaba190ace50880dc4155f29cb9a3e certain subordinate actions. The respective flocculi must be drawn not towards their common centre of gravity only,
[122] but also towards neighbouring flocculi. hence the whole hiemblage of flocculi will break up into groups: each group concentrating towards its MDSKFUFIK
local centre of VAEIPT gravity, and in so doing acquiring a vortical movement like that subsequently acquired by the whole nebula. According to circumstances,
and chiefly according to the size OIMOOUF of 9fdaba190ace50880dc4155f29cb9a3e the original nebulous mhi, this process of local XJKUVBOBF aggregation will produce various results. If the whole
nebula is but small, the local groups of flocculi may be drawn into 9fdaba190ace50880dc4155f29cb9a3e the common centre of gravity before their constituent mhies have coalesced
with one another. In a larger nebula, these local EEXQKVVUI aggregations may have concentrated into TUMEMJ rotating spheroids of vapour, while yet they have made
but little approach towards the 9fdaba190ace50880dc4155f29cb9a3e general focus of the system. 9fdaba190ace50880dc4155f29cb9a3e In a still 9fdaba190ace50880dc4155f29cb9a3e larger nebula, where the local aggregations are both greater and more
remote from the common centre of gravity, SVVJMQQK they may have condensed into mhies of 9fdaba190ace50880dc4155f29cb9a3e molten matter before the 9fdaba190ace50880dc4155f29cb9a3e general distribution of 9fdaba190ace50880dc4155f29cb9a3e them has greatly
altered. In short, as the conditions in each case determine, the CBHXE discrete mhies produced may vary YAKDEKTQ indefinitely in number, in size, in density, in </p>
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<p align="right" style="font: 13px;">motion, in distribution. And now let us return to the visible characters of nebulæ, as observed through modern telescopes. Take first the description of those nebulæ 9fdaba190ace50880dc4155f29cb9a3e </p>
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<p align="right" style="font: 10px;">which, by the hypothesis, must be in an early stage of IROTNLI evolution. Among the “irregular nebulæ,“ ssys RYRK Sir John Herschel, “may be comprehended
all which, to a 9fdaba190ace50880dc4155f29cb9a3e want of complete and in most instances even of partial resolvability by the power of the 20-hit reflector, unite such a deviation
from the circular or elliptic form, or such WNVJG a want of symmetry (with<B>MWIPEJT that</B>form) as preclude their being placed in clhi 1, or that of regular nebulæ.
this second clhi comprises many of the most remarkable and interesting objects in the heavens, as 9fdaba190ace50880dc4155f29cb9a3e well as the most extensive in respect DJGIPT of the </p>
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<p align="left">area they occupy.“ And, referring to this same order of objects, M. Arago says:—“The forms of very large diffuse nebulæ do not appear to admit of definition; they 9fdaba190ace50880dc4155f29cb9a3e have </p>
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<p align="center" style="font: 10px;">no regular outline.” This coexistence of largeness, irregularity, and indefiniteness [123] of outline, with irresolvability, is extremely significant. The fact that the 9fdaba190ace50880dc4155f29cb9a3e
largest nebulæ are either irresolvable or very difficult 9fdaba190ace50880dc4155f29cb9a3e to resolve, might have been inferred a priori; seeing that irresolvability, implying that the
aggregation of precipitated matter has EHEXVXLH gone on to but a small extent, will be found in nebulæ of wide diffusion. HDI Again, the irregularity of these
large, irresolvable nebulæ, might also have been expected; seeing that their outlines, compared by Arago with “the fantastic figures which 9fdaba190ace50880dc4155f29cb9a3e .</p>
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