Rotation curves and scaling relations of extremely massive spiral galaxies

@article{diTeodoro2021RotationCA,
  title={Rotation curves and scaling relations of extremely massive spiral galaxies},
  author={Enrico M di Teodoro and Lorenzo Posti and Patrick M. Ogle and S. Michael Fall and Thomas H. Jarrett},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2021}
}
We study the kinematics and scaling relations of a sample of 43 giant spiral galaxies that have stellar masses exceeding $10^{11} \, {\rm M}_\odot$ and optical discs up to 80 kpc in radius. We use a hybrid 3D–1D approach to fit 3D kinematic models to long-slit observations of the H α-$\rm{[N\, \small {II}]}$ emission lines and we obtain robust rotation curves of these massive systems. We find that all galaxies in our sample seem to reach a flat part of the rotation curve within the outermost… 

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