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Dive into the research topics of 'CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: Dependence on redshift, halo mass, and radius'. Together they form a unique fingerprint.- Sort by
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S. Roca-Fàbrega*, A. Dekel, Y. Faerman, O. Gnat, C. Strawn, D. Ceverino, J. Primack, A. V. Macciò, A. A. Dutton, J. X. Prochaska, J. Stern
Research output: Contribution to journal › Article › peer-review