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  • 1. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/IREvolvePasadenaConfPoster.pdf
    ... studies of a moderate (NGC 520) and very intense (Arp 220) starburst are presented ... fit to the observed spectrum of Arp 220 requires destruction of a large fraction of ... Case study: Arp 220 Spitzer/IRS spectra (solid line) HST/ Thompson 2005 Dust ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/IREvolvePasadenaConfPoster.pdf -- 1225.1 Кб -- 25.11.2009
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    2. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/MidIRSocorroNov05.pdf
    ... 2005: Mid-IR Emission from Galaxies ­ p. 35 Case study II: Arp 220 HST/NICMOS [Thomson et al] UKIRT/MICHELLE SFR: 120 M yr-1 ... Socorro 2005: Mid-IR Emission from Galaxies ­ p. 36 Arp 220 model 100 10 1 F (Jy) 0. 1 0.01 0.001 5 10 20 (µm) 50 100 200 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/MidIRSocorroNov05.pdf -- 1996.8 Кб -- 25.11.2009
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    3. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_thesis.html
    ... radio, near-infrared observations, mid-infrared emission from NGC 520 and Arp 220 is modelled with considerable success ... is significant processing of dust in the extreme radiation field of Arp 220, leading to destruction of most, but not all, dust ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_thesis.html -- 9.5 Кб -- 25.11.2009
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    4. http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-11-02-Cambridge.pdf
    ... 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 Arp 220 I Arp 220 1 · 102 5 · 102 4 2.5 · 10- 3 163 2 · 10- 2 · 102 F (Jy) 1 · 10 3 163 1.5 · 10 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-11-02-Cambridge.pdf -- 1535.6 Кб -- 10.08.2012
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    5. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_MidIRSocorroNov05.html
    ... 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 Arp 220 ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_MidIRSocorroNov05.html -- 8.1 Кб -- 25.11.2009
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    6. http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-JAO-intro.pdf
    ... 100 (GHz) 2 · 109 10 1 · 101 0 5 · 109 1 · 109 (GHz) Z this model is preferred B. Nikolic (Cambridge) Fitting of radio spectra 37 / 75 (U)LIRGs Gallery of fan char ts II Arp 220 0.5 kpc comp + 0.05 kpc comp 600 1 0.5 500 0.2 400 0.1 F (Jy) 0.05 0.02 0.01 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-JAO-intro.pdf -- 1383.5 Кб -- 10.08.2012
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    7. http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-09-Sardinia.pdf
    ... 100 (GHz) 2 · 109 10 1 · 101 0 5 · 109 1 · 109 (GHz) Z this model is preferred B. Nikolic (Cambridge) Fitting of radio spectra 42 / 80 (U)LIRGs Gallery of fan char ts II Arp 220 0.5 kpc comp + 0.05 kpc comp 600 1 0.5 500 0.2 400 0.1 F (Jy) 0.05 0.02 0.01 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-09-Sardinia.pdf -- 1520.2 Кб -- 10.08.2012
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    8. http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02652v3.pdf
    ... 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 Arp 220 (OM13 and references therein). ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02652v3.pdf -- 449.7 Кб -- 04.03.2016
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    9. http://www.mrao.cam.ac.uk/galevol/talk_abstracts.pdf
    ... 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 Arp 220-luminosity galaxies at z > 2. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/galevol/talk_abstracts.pdf -- 226.0 Кб -- 29.08.2013
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    10. Dave Green: Publications
    ... 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 . ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~dag/my-papers.html -- 64.5 Кб -- 30.03.2016
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