The role of active galactic nucleus feedback on the evolution of dwarf galaxies from cosmological simulations - Supermassive black holes suppress star formation in low-mass galaxies

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Volume 690 (October 2024)

A&A, 690 (2024) A286

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Table 1.

z = 0 properties of simulated dwarf galaxies run with and without the inclusion of AGNs.

		AGN				no AGN
ID	Run	$\frac{M_{200}}{(10^{10} M_{⊙})}$ $\frac{M_{200}}{(10^{10} M_\odot)}$	$\frac{R_{200}}{(kpc)}$ $\frac{R_{200}}{(\mathrm{kpc})}$	$\frac{M_{⋆}}{(10^{9} M_{⊙})}$ $\frac{M_\star}{(10^{9} M_\odot)}$	$\frac{M_{BH}}{(10^{6} M_{⊙})}$ $\frac{M_{\mathrm{BH}}}{(10^{6} M_\odot)}$	$\frac{M_{200}}{(10^{10} M_{⊙})}$ $\frac{M_{200}}{(10^{10} M_\odot)}$	$\frac{R_{200}}{(kpc)}$ $\frac{R_{200}}{(\mathrm{kpc})}$	$\frac{M_{⋆}}{(10^{9} M_{⊙})}$ $\frac{M_\star}{(10^{9} M_\odot)}$
Au5	H0	27.44	136.97	5.70	13.34	28.99	139.51	6.58
Au3	H1	21.50	126.27	4.21	9.37	22.53	128.25	5.89
Au1	H2	20.31	123.91	2.74	4.18	21.08	125.45	3.70
Au4	H3	28.62	138.90	2.89	2.76	29.30	140.00	3.65
Au2	H4	12.41	105.13	0.96	1.97	12.94	106.60	1.88
Au0	H5	9.37	95.73	0.69	1.80	9.63	96.61	1.05
Au7	H6	13.84	109.03	1.13	1.67	14.77	111.41	1.82
Au11	H7	7.52	88.96	0.64	1.14	7.90	90.43	0.90
Au6	H8	7.78	90.00	0.78	0.88	7.93	90.56	0.86
Au10	H9	6.54	84.93	0.41	0.41	6.71	85.66	0.50
Au8	H10	9.67	96.74	0.36	0.41	9.84	97.31	0.41
Au9	H11	8.85	93.92	0.24	0.29	8.92	94.19	0.25

Notes. The columns represent: (1) AURIGA ID, (2) run name; and for the sample with AGN, (3) halo virial mass, (4) halo virial radius, (5) stellar mass, and (6) BH mass; and for the sample without AGN, (7) halo virial mass, (8) halo virial radius, and (9) stellar mass.

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