The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
S. Bekerait\.e, C.J. Walcher, J. Falc\'on-Barroso, B. Garcia Lorenzo,, M. Lyubenova, S.F. S\'anchez, K. Spekkens, G. van de Ven, L. Wisotzki, B., Ziegler, J.A.L. Aguerri, J. Barrera-Ballesteros, J. Bland-Hawthorn, Cristina, Catal\'an-Torrecilla, R. Garc\'ia-Benito
TL;DR
This paper presents a volume-complete Tully-Fisher relation derived from CALIFA stellar kinematics, providing insights into galaxy distribution in the magnitude-rotation velocity plane.
Contribution
It introduces a new, volume-complete Tully-Fisher relation based on stellar kinematics from CALIFA, improving galaxy distribution understanding.
Findings
Established a volume-complete galaxy sample
Derived a new Tully-Fisher relation from stellar kinematics
Enhanced understanding of galaxy distribution in magnitude-velocity space
Abstract
The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
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