An analysis of the FIR/RADIO continuum correlation in the small Magellanic cloud
Autor: | Howard Leverenz, Miroslav Filipovic |
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Rok vydání: | 2012 |
Předmět: |
Luminous infrared galaxy
Physics Photon Continuum (design consultancy) FOS: Physical sciences Astronomy and Astrophysics Cosmic ray Electron Astrophysics Astrophysics - Astrophysics of Galaxies Power law Magnetic field Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) Small Magellanic Cloud |
Zdroj: | Astrophysics and Space Science. 343:301-317 |
ISSN: | 1572-946X 0004-640X |
Popis: | The local correlation between far-infrared (FIR) emission and radio-continuum (RC) emission for the Small Magellanic Cloud (SMC) is investigated over scales from 3 kpc to 0.01 kpc. Here, we report good FIR/RC correlation down to ~15 pc. The reciprocal slope of the FIR/RC emission correlation (RC/FIR) in the SMC is shown to be greatest in the most active star forming regions with a power law slope of ~1.14 indicating that the RC emission increases faster than the FIR emission. The slope of the other regions and the SMC are much flatter and in the range of 0.63-0.85. The slopes tend to follow the thermal fractions of the regions which range from 0.5 to 0.95. The thermal fraction of the RC emission alone can provide the expected FIR/RC correlation. The results are consistent with a common source for ultraviolet (UV) photons heating dust and Cosmic Ray electrons (CRe-s) diffusing away from the star forming regions. Since the CRe-s appear to escape the SMC so readily, the results here may not provide support for coupling between the local gas density and the magnetic field intensity. 19 pages, 7 Figures |
Databáze: | OpenAIRE |
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