Physical Parameters of Late Type Spiral Galaxies I-Mass and Luminosity of NGC 6946 [PDF]
Journal of Astronomy and Space Sciences, 1985 Using Brandt model the mass distribution of the late type spiral galaxy NGC 6946 was derived, and the total mass was reestimated to understand the M/L ratio of this galaxy. Two kinds of the rotation curve with shape parameter n = 1 and 3.3 were examined.
Sug-Whan Kim, Mun-Suk Chun
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Spectroscopic Studies of Starburst Galaxies; the Dynamical Structure of Blue Compact Dwarf Galaxy Haro 6 [PDF]
Journal of Astronomy and Space Sciences, 1995 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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The Inner Regions of Disk Galaxies: A Constant Baryonic Fraction?
Galaxies, 2014 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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Nuclear-to-Outer Rotation Curves of Galaxies in the CO and H
, 1997 Yoshiaki Sofue
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Erratum: The universal rotation curve of spiral galaxies -- I. The dark matter connection [PDF]
, 1996 M. Persic, P. Salucci, F. Stel
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Stellar dynamics around transient co-rotating spiral arms
EPJ Web of Conferences, 2012 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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Signatures of Interstellar-Intracluster Medium Interactions: Spiral Galaxy Rotation Curves in Abell 2029 [PDF]
, 2000 Daniel A. Dale, Juan M. Uson
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Interpretation of Rotation Curves of Giant Galaxies in the Local Group with the Truncated Disk Model: the Milky Way [PDF]
, 2000 I. I. Nikiforov +2 more
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An Equilibrium Model of the Galaxy Determined by Element Abundance Gradients
The Astrophysical JournalWe 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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Reanalysis of the MACHO Constraints on PBH in the Light of Gaia DR3 Data
UniverseThe 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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