... studies of a moderate (NGC 520) and very intense (Arp220) starburst are presented ... fit to the observed spectrum of Arp220 requires destruction of a large fraction of ... Case study: Arp220 Spitzer/IRS spectra (solid line) HST/ Thompson 2005 Dust ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/IREvolvePasadenaConfPoster.pdf -- 1225.1 Кб -- 25.11.2009 Похожие документы
... radio, near-infrared observations, mid-infrared emission from NGC 520 and Arp220 is modelled with considerable success ... is significant processing of dust in the extreme radiation field of Arp220, leading to destruction of most, but not all, dust ...
... linearly dependent to SFR and based on the FIR-radio correlation B. Nikolic (Cambridge) Fitting of radio spectra 2 November 2010 54 / 61 Spectra of (U)LIRGs Arp220 I Arp220 1 · 102 5 · 102 4 2.5 · 10- 3 163 2 · 10- 2 · 102 F (Jy) 1 · 10 3 163 1.5 · 10 ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-11-02-Cambridge.pdf -- 1535.6 Кб -- 10.08.2012 Похожие документы
... based on a comprehensive dust model and relatively simple radiative transfer, and illustrate their application to objects in the near-by universe with good multi-wavelength data including some new high resolution mid-infrared imaging (NGC 520 and Arp220 ...
... Taking a value of LI R as in Section 3.2.3, we find an LH 2O /LI R ratio of 6.7в10-6, which is similar to the value found for Arp220 (OM13 and references therein). ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02652v3.pdf -- 449.7 Кб -- 04.03.2016 Похожие документы
... This single-pointing survey has pro duced an image with an RMS noise of 0.5 uJy/beam, which is capable of detecting and resolving Arp220-luminosity galaxies at z > 2. ...
... 2007 : . The unusual distribution of molecular gas and star formation in Arp 140 . ... H I and CO observations of Arp 104: a spiral elliptical interacting pair . ... Green D. A. 1988ASIC..220..205G . ...