@article {2012MNRAS.422..510R,
	title = {{EVN observations of the farthest and brightest ULIRGs in the local Universe: the case of IRAS 23365+3604}},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {422},
	year = {2012},
	month = {may},
	pages = {510-520},
	abstract = {We present high-resolution, high-sensitivity radio images of the ultra-luminous infrared galaxy (ULIRG) IRAS 23365+3604. We performed contemporaneous observations at 1.7 and 5.0 GHz, in three epochs separated by 1 year from each other, with the European Very Long Baseline Interferometry (VLBI) Network (EVN). We also present complementary Multi-Element Radio Linked Interferometry Network (MERLIN) at 1.6 and 5.0 GHz, and archival Very Large Array data, taken at 1.4 and 4.9 GHz. We find that the emission at {\tilde}5.0 GHz remains quite compact as seen at different resolutions, whereas at {\tilde}1.7 GHz, high-resolution imaging reveals some extended structure. The nuclear region has an approximate linear size of 200 pc and shows the presence of two main emission components: (i) one with a composite spectrum due to ongoing non-thermal activity (probably due to recently exploded supernovae and the presence of an active galactic nucleus), and (ii) the other with a steep spectrum, likely dominated by an old population of radio emitters, such as supernova remnants. Radiative losses are important, so re-acceleration or replenishment of new electrons is necessary. We estimate a magnetic field strength of {\tilde} 18 {$μ$}G at galactic and {\tilde} 175 {$μ$}G at nuclear scales, which are typical for galaxies in advanced mergers.},
	keywords = {galaxies: individual: IRAS 23365+3604, galaxies: starburst, radio continuum: general},
	doi = {10.1111/j.1365-2966.2012.20627.x},
	url = {http://adsabs.harvard.edu/abs/2012MNRAS.422..510R},
	author = {Romero-Ca{\~n}izales, C. and M. A. P{\'e}rez-Torres and Alberdi, A.}
}
@article {2011A\&A...535L..10M,
	title = {{VLBI observations of SN 2011dh: imaging of the youngest radio supernova}},
	journal = {Astronomy and Astrophysics},
	volume = {535},
	year = {2011},
	pages = {L10},
	abstract = {We report on the VLBI detection of supernova SN 2011dh at 22 GHz using a subset of the EVN array. The observations took place 14 days after the discovery of the supernova, thus resulting in a VLBI image of the youngest radio-loud supernova ever. We provide revised coordinates for the supernova with milli-arcsecond precision, linked to the ICRF. The recovered flux density is a factor \~{}2 below the EVLA flux density reported by other authors at the same frequency and epoch of our observations. This discrepancy could be due to extended emission detected with the EVLA or to calibration problems in the VLBI and/or EVLA observations.},
	keywords = {ISM: supernova remnants, radiation mechanisms: non-thermal, radio continuum: general, supernovae: general, supernovae: individual: SN 2011dh},
	doi = {10.1051/0004-6361/201118195},
	url = {http://adsabs.harvard.edu/abs/2011A\%26A...535L..10M},
	author = {Mart{\'\i}-Vidal, I. and Tudose, V. and Paragi, Z. and Yang, J. and Marcaide, J.~M. and Guirado, J.~C. and Ros, E. and Alberdi, A. and M. A. P{\'e}rez-Torres and Argo, M.~K. and van der Horst, A.~J. and Garrett, M.~A. and Stockdale, C.~J. and Weiler, K.~W.}
}
