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

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.295..297p&link_type=abstract

Astrophysics and Space Science, Volume 295, Issue 1-2, pp. 297-302

Astronomy and Astrophysics

Astrophysics

Galaxies-Active, Galaxies-Starburst, Galaxies-Nuclei

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 18 cm 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 three galaxies are presented here.

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