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Images

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Images

Global Spectral energy distribution (SED) of NGC 337.

The Herschel filter bandpasses are shown at the bottom of the figure. (Kennicutt et al. 2011)

Spitzer/MIPS and Herschel/PACS 70 and 160 μm maps of the galaxy NGC628.

Note the improvment in terms of spatial resolution between the two instruments. (Kennicutt et al. 2011)

The galaxy NGC628 observed with the Spitzer and Herschel space telescopes.

Top: Spitzer images at 3.6 μm, 8.0 μm and 24 μm. The emissionis dominated by stars, small PAH grains, and small dust grains heated by intense radiatino fields, respectively.
Middle: Herschel PACS images at 70 μm, 100 μm, and 160 μm. Note the progressive increase in contributions from diffuse dust emission with increasing wavelength.
Bottom: Herschel SPIRE images at 250 μm, 350 μm, and 500 μm. These bands trace increasingly cooler components of the main thermal dust emission.

Same for NGC6946 (Kennicutt et al. 2011).

Talks

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Talk for Non-Astronomers, Maud Galametz, ESO Garching, 2015

Visuals

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Interactive KINGFISH Hubble Tuning Fork

Press releases