Supernovae and Star Formation in the ULIRG Arp 220

Details Supernovae and Star Formation in the ULIRG Arp 220 Supernovae and Star Formation in the ULIRG Arp 220

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..200t&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Astronomy and Astrophysics

Astronomy

Scientific paper

For over a decade, the ULIRG Arp 220 has been the object of a high
sensitivity VLBI campaign at a wavelength of 18 cm to observe the
evolution of a cluster of unresolved radio sources, originally
identified as Type IIn radio supernovae by tet{smith1998}. The results
of the most recent VLBI observations of Arp 220 are summarized here.

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