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English: Baryonic Tully-Fisher relation
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Source Own work Data compiled from.[1][2][3][4][5][6]
Author ScienceDawns

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  1. ↑ (2022). "The Cen A galaxy group: Dynamical mass and missing baryons". Astronomy & Astrophysics 662: A57. DOI:10.1051/0004-6361/202142351. ISSN 0004-6361.
  2. ↑ (2021-11-01). "The Baryonic Tully–Fisher Relation in the Local Group and the Equivalent Circular Velocity of Pressure-supported Dwarfs". The Astronomical Journal 162 (5): 202. DOI:10.3847/1538-3881/ac2502. ISSN 0004-6256.
  3. ↑ (2019-04-11). "The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum". Monthly Notices of the Royal Astronomical Society 484 (3): 3267–3278. DOI:10.1093/mnras/stz205. ISSN 0035-8711.
  4. ↑ (2021-09-20). "Rotation curves and scaling relations of extremely massive spiral galaxies". Monthly Notices of the Royal Astronomical Society 507 (4): 5820–5831. DOI:10.1093/mnras/stab2549. ISSN 0035-8711.
  5. ↑ (2024-07-01). "Indefinitely Flat Circular Velocities and the Baryonic Tully–Fisher Relation from Weak Lensing". The Astrophysical Journal Letters 969 (1): L3. DOI:10.3847/2041-8213/ad54b0. ISSN 2041-8205.
  6. ↑ Milgrom, Mordehai (2019-02-20). "MOND in galaxy groups: A superior sample". Physical Review D 99 (4). DOI:10.1103/PhysRevD.99.044041. ISSN 2470-0010.

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Baryonic Tully-Fisher relation

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