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dwarf spiral galaxy : ウィキペディア英語版
dwarf spiral galaxy

A dwarf spiral galaxy is the dwarf version of a spiral galaxy. Dwarf galaxies are characterized as having low luminosities, small diameters (less than 5 kpc), low surface brightnesses, and low hydrogen masses. The galaxies may be considered a subclass of low-surface-brightness galaxies.
Dwarf spiral galaxies, particularly the dwarf counterparts of Sa-Sc type spiral galaxies, are quite rare. In contrast, dwarf elliptical galaxies, dwarf irregular galaxies, and the dwarf versions of Magellanic type galaxies (which may be considered transitory between spiral and irregular in terms of morphology) are very common.〔
It is suggested that dwarf spiral galaxies can transform into dwarf elliptical galaxies, especially in dense cluster environments.〔 〕
==Examples==

* NGC 5474
* NGC 5204
* NGC 247
* NGC 6503
* NGC 3928
* NGC 625
* NGC 1051
* NGC 1311
* NGC 2188
* IC 4710

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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