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The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology
J. Fritz, G. Gentile, M. W. L. Smith +30
We have obtained Herschel images at five wavelengths from 100 to 500 micron of a ~5.5x2.5 degree area centred on the local galaxy M31 (Andromeda), our nearest neighbour spiral gala…
Variation in the dust spectral index across M33
F. S. Tabatabaei, J. Braine, C. Kramer +9
Using the Herschel PACS and SPIRE FIR/submm data, we investigate variations in the dust spectral index in the nearby spiral galaxy M33 at a linear resolution of 160 pc. We use…
Spectral Energy Distributions of a set of HII regions in M33 (HerM33es)
M. Relano, S. Verley, I. Perez +7
Within the framework of the HerM33es Key Project for Herschel and in combination with multi-wavelength data, we study the Spectral Energy Distribution (SED) of a set of HII regions…
Dust heating sources in galaxies: the case of M33 (HERM33ES)
M. Boquien, D. Calzetti, F. Combes +7
Dust emission is one of the main windows to the physics of galaxies and to star formation as the radiation from young, hot stars is absorbed by the dust and reemitted at longer wav…
Studying the spatially resolved Schmidt-Kennicutt law in interacting galaxies: the case of Arp 158
Médéric Boquien, Ute Lisenfeld, Pierre-Alain Duc +4
Recent studies have shown that star formation in mergers does not seem to follow the same Schmidt-Kennicutt (KS) relation as in spiral disks, presenting a higher star formation rat…
The Herschel M33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302
B. Mookerjea, C. Kramer, C. Buchbender +19
Context: The emission line of [CII] at 158 micron is one of the strongest cooling lines of the interstellar medium (ISM) in galaxies. Aims: Disentangling the relative contributions…