The Tully--Fisher relation of cluster spirals at z = 0.83
- 11 February 2003
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 339 (1) , L1-L5
- https://doi.org/10.1046/j.1365-8711.2003.06324.x
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This publication has 16 references indexed in Scilit:
- The Evolution of the Tully-Fisher Relation of Spiral GalaxiesThe Astrophysical Journal, 2002
- Gone with the Wind: The Origin of S0 Galaxies in ClustersScience, 2000
- A High Merger Fraction in the Rich Cluster MS 1054−03 at [CLC][ITAL]z[/ITAL][/CLC] = 0.83: Direct Evidence for Hierarchical Formation of Massive GalaxiesThe Astrophysical Journal, 1999
- The Star Formation Histories of Galaxies in Distant ClustersThe Astrophysical Journal, 1999
- Analysis of Spatially Resolved Emission Lines in the Spectra of Distant GalaxiesPublications of the Astronomical Society of the Pacific, 1999
- Internal Kinematics of Field Galaxies at Intermediate RedshiftsThe Astrophysical Journal, 1998
- Is There a Deficit of S0 Galaxies at Intermediate Redshift?The Astrophysical Journal, 1998
- The relationship between past and present star formation in galactic disks from CCD surface photometryThe Astrophysical Journal, 1994
- Luminosity-line width relations and the extragalactic distance scale. I - Absolute calibrationThe Astrophysical Journal, 1992
- The universal galaxy rotation curveThe Astrophysical Journal, 1991