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Linear relation between H I circular velocity and stellar velocity dispersion in early-type galaxies, and slope of the density profiles

MPS-Authors

Serra,  P.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Oosterloo,  T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Cappellari,  M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

den Heijer,  M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Józsa,  G.I.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Serra, P., Oosterloo, T., Cappellari, M., den Heijer, M., & Józsa, G. (2016). Linear relation between H I circular velocity and stellar velocity dispersion in early-type galaxies, and slope of the density profiles. Monthly Notices of the RAS, 460, 1382-1389. doi:10.1093/mnras/stw1010.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-15BE-5
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