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Relevant bibliographies by topics / Tully-Fisher relation

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Academic literature on the topic 'Tully-Fisher relation'

Author: Grafiati

Published: 14 March 2023

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Journal articles on the topic "Tully-Fisher relation"

1

Tully, Richard. "Tully-Fisher relation." Scholarpedia 2, no. 12 (2007): 4485. http://dx.doi.org/10.4249/scholarpedia.4485.

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2

M. ALI, AKRAM. "TULLY - FISHER RELATION PROOFING." Journal of University of Anbar for Pure Science 3, no. 3 (2009): 177–83. http://dx.doi.org/10.37652/juaps.2009.15642.

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3

Gurovich, Sebastián, Stacy S. McGaugh, Ken C. Freeman, Helmut Jerjen, Lister Staveley-Smith, and W. J. G. De Blok. "The Baryonic Tully–Fisher Relation." Publications of the Astronomical Society of Australia 21, no. 4 (2004): 412–14. http://dx.doi.org/10.1071/as04038.

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AbstractWe validate the baryonic Tully–Fisher (TF) relation by exploring the Tully–Fisher (TF) and BTF properties of optically and Hi-selected disk galaxies. The data includes galaxies from Sakai et al. (2000) calibrator sample, McGaugh et al. (2000: M2000) I-band sample, and 18 newly acquired Hi-selected field dwarf galaxies observed with the ANU 2.3-m telescope and the ATNF Parkes telescope (Gurovich 2005a).As in M2000, we re-cast the TF and BTF relations as relationships between baryon mass and W20. First we report some numerical errors in M2000. Then, we calculate weighted bi-variate linea

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4

McGaugh, S. S., J. M. Schombert, G. D. Bothun, and W. J. G. de Blok. "The Baryonic Tully-Fisher Relation." Astrophysical Journal 533, no. 2 (2000): L99—L102. http://dx.doi.org/10.1086/312628.

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5

Meyer, Martin J., Martin A. Zwaan, Rachel L. Webster, and Stephen E. Schneider. "Tully-Fisher Relations from an HI-Selected Sample." Symposium - International Astronomical Union 220 (2004): 411–12. http://dx.doi.org/10.1017/s0074180900183731.

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The Tully-Fisher relation is of interest because of its use as a secondary distance measure and the constraints it places on the physics of rotationally supported galaxies. We use data from the HI Parkes All-Sky Survey Catalogue to study and apply the Tully-Fisher relation on a sample of galaxies selected on their HI properties. the issues of third parameter dependencies and intrinsic scatter of the Tully-Fisher relation are investigated.

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6

de Oliveira, Claudia Mendes, Sergio Torres-Flores, Philippe Amram, Henri Plana, and Benoit Epinat. "3D Studies of Galaxies in Compact Groups." Proceedings of the International Astronomical Union 10, S309 (2014): 175–77. http://dx.doi.org/10.1017/s1743921314009612.

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AbstractFabry-Perot data of compact group galaxies have been used to show that the Tully-Fisher relation in any photometric band, for galaxies with vmax > 100 km/s, is very similar to that for galaxies in other less dense environments. In the low-luminosity end, however, a few compact group galaxies fall above the relation apparently because they are too bright for their mass. Here we show that if the mass is properly computed from spectral energy distribution fitting or mass modelling, for the low-luminosity galaxies, their positions in the stellar-mass or baryonic Tully-Fisher relation ar

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7

Pfenniger, D., and Y. Revaz. "The Baryonic Tully-Fisher relation revisited." Astronomy & Astrophysics 431, no. 2 (2005): 511–16. http://dx.doi.org/10.1051/0004-6361:20041660.

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8

Andersen, David R., and Matthew A. Bershady. "A Face-on Tully-Fisher Relation." Astrophysical Journal 599, no. 2 (2003): L79—L82. http://dx.doi.org/10.1086/381292.

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9

Ferrero, Ismael, and Mario G. Abadi. "Redshift evolution of Tully-Fisher relation." Proceedings of the International Astronomical Union 11, S321 (2016): 126. http://dx.doi.org/10.1017/s1743921316009054.

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AbstractUsing the eagle cosmological simulation of galaxy formation we test the ability of the ΛCDM cosmological model to reproduce the Tully-Fisher relation (TFR) and its redshift evolution. We find that our simulated galaxies follow a TFR that is in good agreement with observed results up to z = 1, indicating no evolution in the slope and a weak decrease in the zero-point.

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10

Mould, Jeremy, Mingsheng Han, and Greg Bothun. "Nonlinearity of the Tully-Fisher relation." Astrophysical Journal 347 (December 1989): 112. http://dx.doi.org/10.1086/168101.

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