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A physically motivated toy model for the BH-Spheroid coevolution

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Sazonov,  S. Yu.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Ciotti, L., Ostriker, J. P., & Sazonov, S. Y. (2005). A physically motivated toy model for the BH-Spheroid coevolution. In A. Merloni, S. Nayakshin, & R. A. Sunyaev (Eds.), Growing black holes: accretion in a cosmological context (pp. 68-69). Berlin: Springer.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-B3E6-E
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