Cold galaxies

doi:10.1093/mnras/stv1762

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Cold galaxies

2015-08-27

M. Rowan-Robinson *

D. L. Clements

DOI：10.1093/mnras/stv1762

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Abstract

En 中文

We use 350 mu m angular diameter estimates from Planck to test the idea that some galaxies contain exceptionally cold (10-13 K) dust, since colder dust implies a lower surface brightness radiation field illuminating the dust, and hence a greater physical extent for a given luminosity. The galaxies identified from their spectral energy distributions as containing cold dust do indeed show the expected larger 350 mu m diameters. For a few cold dust galaxies where Herschel data are available, we are able to use submillimetre maps or surface brightness profiles to locate the cold dust, which as expected generally lies outside the optical galaxy.

Keywords:

stars: formation

galaxies: evolution

galaxies: starburst

cosmology: observations

infrared: galaxies

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Key information extracted from the uploaded paper, including a brief overview, abstract, background, key highlights, visual analysis, and future outlook.

Journal

Monthly Notices of the Royal Astronomical Society

IF:

4.8

Papers:

7.0W

Citations:

25.0W

Organization

Imperial College London

Scholars:

8.3W

Papers: 7.3W

Citations: 11.1W

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