Connection between dynamically derived initial mass function normalization and 
stellar population parameters

McDermid, Richard M.; Cappellari, Michele; Alatalo, Katherine; Bayet, Estelle; Blitz, Leo; Bois, Maxime; Bournaud, Frédéric; Bureau, Martin; Crocker, Alison F.; Davies, Roger L.; Davis, Timothy A.; de Zeeuw, P. T.; Duc, Pierre-Alain; Emsellem, Eric; Khochfar, Sadegh; Krajnović, Davor; Kuntschner, Harald; Morganti, Raffaella; Naab, Thorsten; Oosterloo, Tom; Sarzi, Marc; Scott, Nicholas; Serra, Paolo; Weijmans, Anne-Marie; Young, Lisa M.

doi:10.1088/2041-8205/792/2/L37

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Connection between dynamically derived initial mass function normalization and stellar population parameters

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Naab, Thorsten
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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McDermid, R. M., Cappellari, M., Alatalo, K., Bayet, E., Blitz, L., Bois, M., et al. (2014). Connection between dynamically derived initial mass function normalization and stellar population parameters. The Astrophysical Journal Letters, 792(2): L37. doi:10.1088/2041-8205/792/2/L37.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0023-F782-1

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