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Dark matter in spiral galaxies
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1986Abstract Mass models of spiral galaxies based on the observed light distribution, assuming constant M /L for bulge and disc, are able to reproduce the observed rotation curves in the inner regions, but fail to do so increasingly towards and beyond the edge of the visible material.
VANALBADA, TS, SANCISI, R
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Are There Jets in Spiral Galaxies?
1983The absence in spiral galaxies of large-scale collimated jets of radio emission is still little understood. Collimated emission in elliptical galaxies in some cases exceeds by far the optical extent of the galaxy (e.g. in NGC6251). Westerbork observations of NGC4258 (van der Kruit, Oort and Mathewson, 1972) and NGC3079 (de Bruyn, 1977) have provided ...
C. Kotanyi, E. Hummel, J. van Gorkom
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Comparison of the Galaxy with External Spiral Galaxies
1987In this chapter some areas of comparative exploration in our and external galaxies are reviewed and discussed. Photometric parameters for the Galaxy are derived. The radial scalelength is 5.0 ± 0.5 kpc, and this makes our Galaxy (and M31) unusually large unless Ho = 65 ± 10 km s−1 Mpc−1. Surface photometry of external edge-on galaxies, in particular of
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Galaxies decomposition with spiral arms – I: 29 galaxies from S4G
Monthly Notices of the Royal Astronomical Society, 2023Aleksandr Mosenkov +2 more
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Rotation curves and scaling relations of extremely massive spiral galaxies
Monthly Notices of the Royal Astronomical Society, 2021Lorenzo Posti +2 more
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Spiral structure in nearby galaxies - I. Sample, data analysis and overview of results
Monthly Notices of the Royal Astronomical Society, 2011Clarke C, Kennicutt R C
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What determines the sizes of bars in spiral galaxies?
Monthly Notices of the Royal Astronomical Society, 2019Peter Erwin, Erwin Peter
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