The shapes of the rotation curves of star-forming galaxies over the last ≈10 Gyr

We analyse maps of the spatially resolved nebular emission of ≈1500 star-forming galaxies at z ≈ 0.6–2.2 from deep K-band Multi-Object Spectrograph and MUSE observations to measure the average shape of their rotation curves. We use these to test claims for declining rotation curves at large radii in...

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Bibliographic Details
Main Authors:	Tiley, A, Swinbank, A, Harrison, C, Smail, I, Turner, O, Schaller, M, Stott, J, Sobral, D, Theuns, T, Sharples, R, Gillman, S, Bower, R, Bunker, A, Best, P, Richard, J, Bacon, R, Bureau, M, Cirasuolo, M, Magdis, G
Format:	Journal article
Published:	Oxford University Press 2019

The shapes of the rotation curves of star-forming galaxies over the last ≈10 Gyr

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