An Explanation for the Observed Weak Size Evolution of Disk Galaxies by Somerville, R, Barden, M, Rix, H, Bell, E, Beckwith, S, Borch, A, Caldwell, J, Haeussler, B, Heymans, C, Jahnke, K, Jogee, S, McIntosh, D, Meisenheimer, K, Peng, C, Sanchez, S, Wisotzki, L, Wolf, C

“…Similarly, we predict that the rotation velocity at a given stellar mass (essentially the zero-point of the Tully-Fisher relation) is only about 10 percent larger at z~1 (20 percent at z~2) than at the present day.…”

The Spectroscopy and H-band Imaging of Virgo Cluster Galaxies (SHIVir) survey: Scaling relations and the stellar-to-total mass relation by Ouellette, N, Courteau, S, Holtzman, J, Dutton, A, Cappellari, M, Dalcanton, J, McDonald, M, Roediger, J, Taylor, J, Tully, R, Côté, P, Ferrarese, L, Peng, E

“…An analysis of the Tully-Fisher relation (TFR) of late-type galaxies (LTGs) and fundamental plane (FP) of early-type galaxies (ETGs) is also presented, yielding a compendium of galaxy scaling relations. …”

Parameterized Asymmetric Neutral Hydrogen Disk Integrated Spectrum Characterization (PANDISC). I. Introduction to a Physically Motivated H i Model by Bo Peng, Martha P. Haynes, Catie J. Ball, Michael G. Jones

“…The model is also shown to be useful for applications like the baryonic Tully–Fisher relation (BTFR) and profile-based sample control. …”
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The Logotropic Dark Fluid as a unification of dark matter and dark energy by Pierre-Henri Chavanis

“…It also implies the Tully–Fisher relation Mb/vh4=44M⊙km−4s4. We stress that our model has no free parameter.…”
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On the Incompleteness of Birkhoff’s Theorem: A New Approach to the Central Symmetric Gravitational Field in Vacuum Space by Michel Canac

“…This 4-metric is thus in agreement with the baryonic Tully–Fisher relation (BTFR), (consequently BTFR is in agreement with a solution of General Relativity without presence of dark matter and without hypothesis on the distribution of stars in galaxies). …”
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The Spectroscopy and H-band Imaging of Virgo Cluster Galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-total Mass Relation by Ouellette, Nathalie N.-Q., Courteau, Stéphane, Holtzman, Jon A., Dutton, Aaron A., Cappellari, Michele, Dalcanton, Julianne J., Roediger, Joel C., Taylor, James E., Tully, R. Brent, Côté, Patrick, Ferrarese, Laura, Peng, Eric W., McDonald, Michael A.

“…An analysis of the Tully-Fisher relation (TFR) of late-type galaxies (LTGs) and the fundamental plane (FP) of early-type galaxies (ETGs) is presented, yielding a compendium of galaxy scaling relations. …”
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The ATLAS(3D) Project - XIV. The extent and kinematics of the molecular gas in early-type galaxies by Davis, T, Alatalo, K, Bureau, M, Cappellari, M, Scott, N, Young, L, Blitz, L, Crocker, A, Bayet, E, Bois, M, Bournaud, F, Davies, R, de Zeeuw, P, Duc, P, Emsellem, E, Khochfar, S, Krajnovic, D, Kuntschner, H, Lablanche, P, McDermid, R, Morganti, R, Naab, T, Oosterloo, T, Sarzi, M, Serra, P

“…We confirm that the molecular gas reaches beyond the turnover of the circular velocity curve in~70 per cent of our CO-rich ATLAS3D ETGs, validating previous work on the CO Tully-Fisher relation. In general we find that in most galaxies the molecular gas is dynamically cold, and the observed CO rotation matches well model predictions of the circular velocity. …”

Closing the Gap between Observed Low-mass Galaxy H i Kinematics and Cold Dark Matter Predictions by Amy Sardone, Annika H. G. Peter, Alyson M. Brooks, Jane Kaczmarek

“…We also measure baryonic masses and place these on the baryonic Tully–Fisher relation (BTFR). Again, our deepest measurements approach the theoretical predictions for the low-mass end of this relation, a significant improvement on similar measurements based on line widths measured at 50% and 20% of the peak. …”
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Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe by Vogelsberger, Mark, Genel, Shy, Springel, Volker, Torrey, Paul, Sijacki, Debora, Xu, Dandan, Snyder, Greg, Nelson, Dylan, Hernquist, Lars

“…The internal velocity structure of selected well-resolved disc galaxies obeys the stellar and baryonic Tully–Fisher relation together with flat circular velocity curves. …”
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Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND by Valentina Cesare

“…For example, some very tight relations between the properties of dark and baryonic matters in disk galaxies, such as the baryonic Tully–Fisher relation (BTFR), the mass discrepancy–acceleration relation (MDAR), and the radial acceleration relation (RAR), which see the emergence of the acceleration scale <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>a</mi><mn>0</mn></msub><mo>≃</mo><mn>1.2</mn><mo>×</mo><msup><mn>10</mn><mrow><mo>−</mo><mn>10</mn></mrow></msup></mrow></semantics></math></inline-formula> m s<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mrow><mo>−</mo><mn>2</mn></mrow></msup></semantics></math></inline-formula>, cannot be intuitively explained by the CDM paradigm, where cosmic structures form through a stochastic merging process. …”
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Almost Optically Dark Galaxies in DECaLS (I): Detection, Optical Properties, and Possible Origins by Lin Du, Wei Du, Cheng Cheng, Ming Zhu, Haiyang Yu, Hong Wu

“…They deviate from the scaling relations between H i and optical properties defined by the ALFALFA sample and the baryonic Tully–Fisher relation. They agree well with the main sequence of star-forming galaxies but exhibit low star-forming efficiency. …”
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Global Dynamic Scaling Relations of H i-rich Ultra-diffuse Galaxies by Hui-Jie Hu, Qi Guo, Zheng Zheng, Hang Yang, Chao-Wei Tsai, Hong-Xin Zhang, Zhi-Yu Zhang

“…The baryonic Tully–Fisher relation (BTFR), which connects the baryonic mass of galaxies with their circular velocities, has been validated across a wide range of galaxies, from dwarf galaxies to massive galaxies. …”
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Possible Effects of the Fractal Distribution of Relic Wormholes by Alexander A. Kirillov, Elena P. Savelova, Polina O. Vladykina

“…That is the nature of dark matter phenomena, the origin of Faber-Jackson and Tully-Fisher relations and the observed deficit of baryons. …”
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A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations by Genel, Shy, Bryan, Greg L., Springel, Volker, Hernquist, Lars, Nelson, Dylan, Pillepich, Annalisa, Weinberger, Rainer, Pakmor, Rüdiger, Marinacci, Federico, Vogelsberger, Mark

“…Importantly, we compare the macroscopic differences between shadow galaxies to the overall scatter in various galaxy scaling relations, and conclude that, for the star formation-mass and the Tully-Fisher relations, the butterfly effect in our simulations contributes significantly to the overall scatter. …”
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Constraining dark matter halo properties using lensed Supernova Legacy Survey supernovae by Jönsson, J, Sullivan, M, Hook, I, Basa, S, Carlberg, R, Conley, A, Fouchez, D, Howell, D, Perrett, K, Pritchet, C

“…We further find that the normalization of the velocity dispersion of passive and star-forming galaxies are consistent with empirical Faber-Jackson and Tully-Fisher relations, respectively. If we make no assumption on the normalization of these relations, we find that the data prefer gravitational lensing at the 92 per cent confidence level. …”