A low-luminosity type-1 QSO sample - II. Tracing circumnuclear star formation in HE 1029-1831 with SINFONI

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Table 1

Comparison of the nearest Seyfert-1 galaxy NGC 3227, our source HE 1029-1831, and the nearest quasar 3C 273.

Source	Redshift	Scale	Resolution^*	log (L_bol [W])	log (M_BH [M_⊙])	λ_Edd


NGC 3227	0.004	100 pc /″	13 pc	36.86	7.64	0.013
HE 1029-1831	0.0404	800 pc /″	110 pc	37.6	7.2	0.3
3C 273	0.158	3150 pc /″	410 pc	39.94	8.95	0.8

Notes. The redshift is taken from the NED database. Black hole mass and bolometric luminosity of NGC 3227 and 3C 273 are from Woo & Urry (2002) and references therein.

^(*)

Assuming a resolution of such as we reach with AO correction in our observations with the 3″ × 3″ FOV.

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