Continuum EVN and MERLIN Observations of Ultra Luminous Infrared Galaxies

Details Continuum EVN and MERLIN Observations of Ultra Luminous Infrared Galaxies Continuum EVN and MERLIN Observations of Ultra Luminous Infrared Galaxies

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..783..361p&link_type=abstract

THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP Conference Proceedings, Volume 783, pp. 361-366 (2

Astronomy and Astrophysics

Astronomy

Galaxies, Radiosources (Astronomical), Imaging, Galactic Nuclei, Supernova Remnants, Starburst Galaxies And Infrared Excess Galaxies, Galactic Nuclei, Circumnuclear Matter, And Bulges, Supernova Remnants

Scientific paper

Radio imaging of ULIR galaxies is ideal to explore the connection between the starburst and the AGN phenomenon since it is unaffected by dust obscuration, and provides the required high angular resolution to distinguish between an AGN and starburst emission. We have made combined 18cm radio continuum, EVN and MERLIN observations of 13 ULIRGs that have the parsec and deci-parsec scale resolution necessary to distinguish between an AGN and supernovae remnants at the centres of these galaxies, and assess the contribution of each to the total energy distribution. Images of four galaxies are presented here.

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