Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
We present a study of 107 galaxies, groups, and clusters spanning ∼3 orders of magnitude in mass, ∼5 orders of magnitude in central galaxy star formation rate (SFR), ∼4 orders of magnitude in the classical cooling rate () of the intracluster medium (ICM), and ∼5 orders of magnitude in the central bl...
| Autori principali: | , , , |
|---|---|
| Altri autori: | |
| Natura: | Articolo |
| Lingua: | English |
| Pubblicazione: |
American Astronomical Society
2020
|
| Accesso online: | https://hdl.handle.net/1721.1/125311 |