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...
| المؤلفون الرئيسيون: | , , , , , , , , , , , , , , , , , , |
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| التنسيق: | Journal article |
| منشور في: |
Oxford University Press
2019
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