EVN observations of the Ultra Luminous Infrared Galaxies IRAS 23365+3604 and IRAS 07251-0248

dc.creatorRomero-Cañizales, Cristina
dc.creatorPérez-Torres, Miguel Ángel
dc.creatorAlberdi, Antxon
dc.date2008-12-03
dc.date.accessioned2026-07-07T12:08:49Z
dc.date.available2026-07-07T12:08:49Z
dc.descriptionWe present high-sensitivity, high-resolution images of the Ultraluminous Infrared Galaxies (ULIRG; L$_{\mathrm{FIR}} > 10^{12}$ L$_\odot$) IRAS 23365+3604 and IRAS 07251-0248, taken with the EVN at 6 and 18 cm. The images show a large number of compact components, whose luminosities are typical of Type IIL and Type IIn Radio Supernovae (RSNe). Further observations of these ULIRGs will allow us to confirm, or to rule out, their nature. The present observations are part of a project that should result in a significant number of SN detections, providing a direct measurement of the Core Collapse Superova (CCSN) rate and allowing us to estimate the Star Formation Rate (SFR) in our sample of ULIRGs .
dc.description3 pages, 6 figures and 1 table; needs PoS.cls. To be be published in Proceedings of Science, proceedings of The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting, September 23-26, 2008, Bologna, Italy
dc.identifierhttps://arxiv.org/abs/0812.0760
dc.identifierhttp://arxiv.org/abs/0812.0760
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/209454
dc.subjectAstrophysics
dc.titleEVN observations of the Ultra Luminous Infrared Galaxies IRAS 23365+3604 and IRAS 07251-0248
dc.typetext

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