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27 April 2024 |
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Starburst or Seyfert? Adding a radio and far-infrared perspective to the investigation of activity in composite galaxies | | Tanya L. Hill
; Charlene A. Heisler
; Ray P. Norris
; John E. Reynolds
; Richard W. Hunstead
; | | Date: |
16 Sep 2000 | | Subject: | astro-ph | | Affiliation: | School of Physics, University of Sydney, Research School for Astronomy and Astrophysics, Australian National University, Australia Telescope National Facility | | Abstract: | It was once common to regard Seyfert and starburst galaxies as completely different types of object, but there is growing recognition that these classifications refer to the extremes of a continuous spectrum of galaxy types. In a previous study we investigated a sample of galaxies with ambiguous optical emission-line ratios and concluded from near-infrared spectroscopic observations that the sample consisted of composite galaxies, containing both a starburst and an active galactic nucleus (AGN). We now extend our study using radio synthesis and long-baseline interferometer observations made with the Australia Telescope, together with far-infrared IRAS observations, to discuss the relative contribution of starburst and AGN components to the overall luminosity of the composite galaxies. We find that only a small fraction of the radio emission (<10%) can be attributed to an AGN, and that the majority of the far-infrared emission (>90%) is probably due to the starburst component. We also show that an AGN contribution to the optical emission of as little as 10% is sufficient to account for the ambiguous line-ratio diagnostics. | | Source: | arXiv, astro-ph/0009260 | | Services: | Forum | Review | PDF | Favorites | |
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