The near-IR and milliarcsec radio structure of PKS 1345 + 125

Details The near-IR and milliarcsec radio structure of PKS 1345 + 125 The near-IR and milliarcsec radio structure of PKS 1345 + 125

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.256p...6s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 256, no. 1, May 1, 1992, p. 6P-10P. Research supported

Astronomy and Astrophysics

Astronomy

15

Astronomical Photometry, Galactic Nuclei, Infrared Sources (Astronomy), Near Infrared Radiation, Radio Astronomy, Seyfert Galaxies, Galactic Structure, Infrared Astronomy Satellite, Luminosity, Radio Emission, Spatial Resolution

Scientific paper

Near-IR photometry at high spatial resolution and six cm radio observations of the central regions of the Seyfert galaxy PKS 1345 + 125, which is a radio-loud and an ultraluminous IRAS system, is presented. The radio structure is resolved into a linear feature misaligned by about 49 deg with respect to the position angle defining the two near-IR nuclei. This indicates that the previously observed optical line emission within the western Seyfert nucleus is not due to any narrow-line area or extended narrow-line area associated with the radio elliptical, therefore distinguishing PKS 1345 + 125 from archetypal double-nucleus Seyferts.

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