The KMOS^3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6 - 2.7

Autor:	Schreiber, N. M. Förster, Übler, H., Davies, R. L., Genzel, R., Wisnioski, E., Belli, S., Shimizu, T., Lutz, D., Fossati, M., Herrera-Camus, R., Mendel, J. T., Tacconi, L. J., Wilman, D., Beifiori, A., Brammer, G., Burkert, A., Carollo, C. M., Davies, R. I., Eisenhauer, F., Fabricius, M., Lilly, S. J., Momcheva, I., Naab, T., Nelson, E. J., Price, S., Renzini, A., Saglia, R., Sternberg, A., van Dokkum, P., Wuyts, S.
Rok vydání:	2018
Předmět:	Astrophysics - Astrophysics of Galaxies
Druh dokumentu:	Working Paper
DOI:	10.3847/1538-4357/ab0ca2
Popis:	We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.611.2 galaxies. The incidence, strength, and velocity of AGN-driven winds strongly correlates with stellar mass and central concentration. Their outflowing ionized gas appears denser (n_e~1000 cm^-3), and possibly compressed and shock-excited. These winds have comparable mass loading factors as the SF-driven winds but carry ~10 (~50) times more momentum (energy). The results confirm our previous findings of high duty cycle, energy-driven outflows powered by AGN above the Schechter mass, which may contribute to star formation quenching. Comment: Accepted for publication by the The Astrophysical Journal. 36 pages, 13 Figures
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1807.04738 Zobrazit plný text záznamu View this record from Arxiv