The Inner Regions of Disk Galaxies: A Constant Baryonic Fraction?
For disk galaxies (spirals and irregulars), the inner circular-velocity gradient dRV0 (inner steepness of the rotation curve) correlates with the central surface brightness ∑*,0 with a slope of ~0.5.
Federico Lelli
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Spectroscopic Studies of Starburst Galaxies; the Dynamical Structure of Blue Compact Dwarf Galaxy Haro 6 [PDF]
We carried out photometric and spectroscopic observations of the blue compact dwarf galaxy Haro 6 in the Virgo Cluster of Galaxies. The long-slit spectroscopy was employed at three position angles, ϕ = 0°, ϕ = 30°, and ϕ = 120° CCD camera mounted on the ...
Mun-Suk Chun+2 more
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Nuclear-to-Outer Rotation Curves of Galaxies in the CO and H
Yoshiaki Sofue
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Stellar dynamics around transient co-rotating spiral arms
Spiral density wave theory attempts to describe the spiral pattern in spiral galaxies in terms of a long-lived wave structure with a constant pattern speed in order to avoid the winding dilemma.
Cropper M., Grand R.J.J., Kawata D.
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Erratum: The universal rotation curve of spiral galaxies -- I. The dark matter connection [PDF]
M. Persic, P. Salucci, F. Stel
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Signatures of Interstellar-Intracluster Medium Interactions: Spiral Galaxy Rotation Curves in Abell 2029 [PDF]
Daniel A. Dale, Juan M. Uson
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Reanalysis of the MACHO Constraints on PBH in the Light of Gaia DR3 Data
The recent astrometric data of hundreds of millions of stars from Gaia DR3 has allowed for a precise determination of the Milky Way rotation curve up to 28 kpc. The data suggest a rapid decline in the density of dark matter beyond 19 kpc.
Juan García-Bellido, Michael Hawkins
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An Equilibrium Model of the Galaxy Determined by Element Abundance Gradients
We present a method to determine the gravitational potential of the Milky Way from measurements of the locations, velocities, and element abundances of stars in the Galactic disk.
Lawrence M. Widrow+4 more
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Interpretation of Rotation Curves of Giant Galaxies in the Local Group with the Truncated Disk Model: the Milky Way [PDF]
I. I. Nikiforov+2 more
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Precision Velocity Fields in Spiral Galaxies. II. Rotation Curves [PDF]
Charles Beauvais, G. D. Bothun
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