In this theory poster contribution I discuss how the known flattening of spiral-galaxy rotation curves is natural if, outside the galaxy's center, the gravitational potential corresponds to that of a filament, string or otherwise cylindrical structure perpendicular to the galactic plane. While observational evidence and simulations for filamentary structure at larger scales seem solid, it is less clear at scales commensurable with galactic sizes. If nevertheless the hypothesis of an at least partially filamentary source of gravity is temptatively adopted for spiral galaxies, the exponent of the baryonic Tully-Fisher relation due to accretion of visible matter by the filament comes out to reasonably be 4. At a minimum, given this exact analy...
We obtain more straightforwardly some features of dark matter distribution in the halos of galaxies ...
We present decompositions of the rotation curves of three spiral galaxies at redshifts $z \sim$ 0.7...
We investigate the possibility that the observed flatness of the rotation curves of spiral galaxies ...
The flattening of spiral-galaxy rotation curves is unnatural in view of the expectations from Kepler...
The dark matter hypothesis, which is not called into question here, explains why typical rotation cu...
The information contained in galactic rotation curves is examined under a minimal set of assumptions...
Galactic rotation curve is a powerful indicator of the state of the gravitational field within a gal...
After explaining the motivation for this article, we briefly recapitulate the methods used to determ...
Higher order curvature gravity has recently received a lot of attention due to the fact that it give...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
Extensive and meticulous observations of the rotation curves of galaxies show that they are either f...
We discuss the role of the galactic disc in the interpretation of the circular velocities of spiral ...
The deviation of a galaxy from exhibiting a Keplerian curve either indicates the presence of dark ma...
We review the topic of rotation curves of spiral galaxies emphasizing the standard interpretation as...
I will present work from the UK KMOS team showing the extended average rotation curves (out to ~13kp...
We obtain more straightforwardly some features of dark matter distribution in the halos of galaxies ...
We present decompositions of the rotation curves of three spiral galaxies at redshifts $z \sim$ 0.7...
We investigate the possibility that the observed flatness of the rotation curves of spiral galaxies ...
The flattening of spiral-galaxy rotation curves is unnatural in view of the expectations from Kepler...
The dark matter hypothesis, which is not called into question here, explains why typical rotation cu...
The information contained in galactic rotation curves is examined under a minimal set of assumptions...
Galactic rotation curve is a powerful indicator of the state of the gravitational field within a gal...
After explaining the motivation for this article, we briefly recapitulate the methods used to determ...
Higher order curvature gravity has recently received a lot of attention due to the fact that it give...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
Extensive and meticulous observations of the rotation curves of galaxies show that they are either f...
We discuss the role of the galactic disc in the interpretation of the circular velocities of spiral ...
The deviation of a galaxy from exhibiting a Keplerian curve either indicates the presence of dark ma...
We review the topic of rotation curves of spiral galaxies emphasizing the standard interpretation as...
I will present work from the UK KMOS team showing the extended average rotation curves (out to ~13kp...
We obtain more straightforwardly some features of dark matter distribution in the halos of galaxies ...
We present decompositions of the rotation curves of three spiral galaxies at redshifts $z \sim$ 0.7...
We investigate the possibility that the observed flatness of the rotation curves of spiral galaxies ...