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Effective radius : ウィキペディア英語版
Effective radius

The effective radius (R_e) of a galaxy is the radius at which half of the total light of the system is emitted.〔(【引用サイトリンク】url=http://astronomy.swin.edu.au/cms/astro/cosmos/h/Half-light+Radius )〕 This assumes the galaxy has either intrinsic spherical symmetry or is at least circularly symmetric as viewed in the plane of the sky. Alternatively, a half-light contour, or isophote, may be used for spherically and circularly asymmetric objects.
R_e is an important length scale in de Vaucouleurs \sqrt() R law, which characterizes a specific rate at which surface brightness decreases as a function of radius:
:
I(R) = I_e \cdot e^

where I_e is the surface brightness at R = R_e. At R = 0,
:
I(R=0) = I_e \cdot e^ \approx 2000 \cdot I_e

Thus, the central surface brightness is approximately 2000 \cdot I_e.
==See also==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Effective radius」の詳細全文を読む



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