The variable UV central spike of NGC 4552
ASTR SOC P 117 (1997) 545-549
Abstract:
The nature of the UV-bright spike at the center of the otherwise normal galaxy NGC 4552 is investigated by means of both Hubble Space Telescope (HST) imaging (FOC) and spectroscopy (FOS). This central feature-which underwent a recent dramatic UV flare-provides a potential new tool for revealing the presence of massive black holes in normal galaxies. In particular the sub-arcsec FOS spectra of the nucleus suggest that NGC 4552 does harbor an object with mass M > 4 x 10(8) M. within the central 2 pc.Optical and infrared investigation towards the z=3.8 quasar pair PC1643+4631A&B
(1996)
A radio galaxy at redshift 4.41
Nature Springer Nature 383:6600 (1996) 502-505
A New I-Band Tully-Fisher Relation for the Fornax Cluster: Implication for the Fornax Distance and Local Supercluster Velocity Field
The Astrophysical Journal American Astronomical Society 463 (1996) 60