Accretion, radial flows and abundance gradients in spiral galaxies

Accretion, radial flows and abundance gradients in spiral galaxies

The metal-poor gas continuously accreting on to the discs of spiral galaxies is unlikely to arrive from the intergalactic medium (IGM) with exactly the same rotation velocity as the galaxy itself and even a small angular momentum mismatch inevitably drives radial gas flows within the disc, with sign...

書誌詳細
主要な著者:	Pezzulli, G, Fraternali, F
フォーマット:	Journal article
出版事項:	Oxford University Press 2016

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