Faint blue galaxy
The faint blue galaxy (F.B.G.) problem in astrophysics first arose with observations starting in 1978 that there were more galaxies with a bolometric magnitude > 22 than then-current theory predicted. Galaxies can appear faint because they are small or because they are far away. Neither explanation, nor any combination, initially matched the observations. The distribution of these galaxies has since been found to be consistent with Cosmic inflation, measurements of the Cosmic Microwave Background, and a nonzero cosmological constant, that is, with the existence of the now-accepted dark energy. It thus serves as a confirmation of supernova observations requiring dark energy.
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Faint blue galaxy
The faint blue galaxy (F.B.G.) problem in astrophysics first arose with observations starting in 1978 that there were more galaxies with a bolometric magnitude > 22 than then-current theory predicted. Galaxies can appear faint because they are small or because they are far away. Neither explanation, nor any combination, initially matched the observations. The distribution of these galaxies has since been found to be consistent with Cosmic inflation, measurements of the Cosmic Microwave Background, and a nonzero cosmological constant, that is, with the existence of the now-accepted dark energy. It thus serves as a confirmation of supernova observations requiring dark energy.
has abstract
The faint blue galaxy (F.B.G.) ...... by merger with other galaxies.
@en
Une galaxie bleu pâle (en angl ...... ondant dans d'autres galaxies.
@fr
暗藍星系 (Faint blue galaxy,F.B.G. ...... 們中有些通過與其它星系的合併,不再是獨立的天體,因而消失了。
@zh
Wikipage page ID
Wikipage revision ID
708,876,514
subject
comment
The faint blue galaxy (F.B.G.) ...... vations requiring dark energy.
@en
Une galaxie bleu pâle (en angl ...... ondant dans d'autres galaxies.
@fr
暗藍星系 (Faint blue galaxy,F.B.G. ...... 們中有些通過與其它星系的合併,不再是獨立的天體,因而消失了。
@zh
label
Faint blue galaxy
@en
Galaxie bleu pâle
@fr
暗藍星系
@zh