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A Lyman-alpha emitter (LAE) is a type of distant galaxy that emits Lyman-alpha radiation. LAEs are extremely distant, and because of the finite travel time of light they provide glimpses into the history of the universe. They are thought to be the progenitors of most modern Milky Way type galaxies. These galaxies can be found nowadays rather easily in narrow-band searches by an excess of their narrow-band flux at a wavelength which may be interpreted as their redshift: : where z is the redshift, is the observed wavelength, and 1215.67 Å is the wavelength of Lyman-alpha emission. The Lyman-alpha line is thought to be caused by an ongoing outburst of star-formation. Experimental observations of the redshift of LAEs are important in cosmology because they trace dark matter halos and subsequently the evolution of matter distribution in the universe. == Properties == Lyman-alpha emitters are typically low mass galaxies of 10^8 or 10^10 solar masses. They are typically young galaxies that are 200 to 600 Megayears old, and they have the highest specific star formation rate of any galaxies known. All of these properties indicate that Lyman-alpha emitters are important clues as to the progentiors of modern Milky Way type galaxies. Lyman-alpha emitters have many unknown properties. The Lyman-alpha photon escape fraction varies greatly in these galaxies. This is what portion of the light emitted at the Lyman-alpha line wavelength inside the galaxy actually escapes and will be visible to distant observers. There is much evidence that the dust content of these galaxies could be significant and therefore is obscuring the brightness of these galaxies. It is also possible that anisotropic distribution of hydrogen density and velocity play a significant role in the varying escape fraction due to the photons' continued interaction with the hydrogen gas (radiative transfer).〔() Anisotropic Lyman-alpha Emission〕 Evidence now shows strong evolution in the Lyman Alpha escape fraction with redshift, most likely associated with the buildup of dust in the es. It is also possible that anisotropic distribution of hydrogen density and velocity play a significant role in the varying escape fraction due to the photons' continued interaction with the hydrogen gas (radiative transfer).〔() Anisotropic Lyman-alpha Emission〕 Evidence now shows strong evolution in the Lyman Alpha escape fraction with redshift, most likely associated with the buildup of dust in the ISM. Dust is shown to be the main parameter setting the escape of Lyman Alpha photons.〔() HETDEX: Evolution of Lyman Alpha Emitters〕 Additionally the metallicity, outflows, and detailed evolution with redshift is unknown. 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「Lyman-alpha emitter」の詳細全文を読む スポンサード リンク
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