ISO-SWS Results on Ultraluminous IRAS Galaxies
Chapter in Quasar Hosts, Springer Nature (1997) 242-247
Infrared to Millimeter Spectroscopy and Imaging of Active Galactic Nuclei
International Astronomical Union Colloquium Cambridge University Press (CUP) 159 (1997) 312-324
Millimetre line CO (2->1) observations of a complete sample of AGN
ASTRONOMY & ASTROPHYSICS 327:2 (1997) 493-502
NIR imaging spectroscopy of IRAS F10214+4724: Evidence for a starburst region around an AGN at z=2.3
REV MEX AST ASTR 6 (1997) 48-51
Abstract:
We report 1'' K-band imaging spectroscopy of the z=2.284 galaxy IRAS F10214+4724. We find that the rest-frame H alpha and [N II] emission have different spatial extents. Furthermore, we detect broad (Delta upsilon(FWZP)approximate to 3500 km s(-1)) H alpha emission. We conclude that F10214+4724 is a very luminous gravitationally lensed galaxy, which intrinsically contains both a type 1 AGN and a more extended star-forming disk. The AGN and circumnuclear star formation both contribute significantly to the total luminosity of similar to 10(13)L(circle dot).Near-Infrared Imaging Spectroscopy of the Seyfert Nucleus of the Circinus Galaxy
International Astronomical Union Colloquium Cambridge University Press (CUP) 159 (1997) 351-352