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Spectral Energy Distributions of a set of H ii regions in M33 (HerM33es)

Published online by Cambridge University Press:  17 August 2012

Monica Relaño
Affiliation:
Dept. de Física Teórica y del Cosmos, Universidad de Granada, Spain email: mrelano@ugr.es
Simon Verley
Affiliation:
Dept. de Física Teórica y del Cosmos, Universidad de Granada, Spain email: mrelano@ugr.es
Isabel Pérez
Affiliation:
Dept. de Física Teórica y del Cosmos, Universidad de Granada, Spain email: mrelano@ugr.es
Carsten Kramer
Affiliation:
Instituto de Radioastronomía Milimétrica, Granada, Spain
Manolis Xilouris
Affiliation:
Institute of Astronomy and Astrophysics, NOA, Athens, Greece
Médéric Boquien
Affiliation:
Laboratoire d'Astrophysique de Marseille, Marseille, France
Jonathan Braine
Affiliation:
Laboratoire d'Astrophysique de Bordeaux, France
Daniela Calzetti
Affiliation:
Deparment of Astronomy, University of Massachusetts, USA
Christian Henkel
Affiliation:
MPI für Radioastronomie, Bonn, Germany
Corresponding
E-mail address:
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Abstract

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 H ii regions in the Local Group Galaxy M33. Using the Hα emission, we perform a classification of a selected H ii region sample in terms of morphology, separating the objects in filled, mixed, shell and clear shell objects. We obtain the SED for each H ii region as well as a representative SED for each class of objects. We also study the emission distribution of each band within the regions. We find different trends in the SEDs for each morphological type that are related to properties of the dust and their associated stellar cluster. The emission distribution of each band within the region is different for each morphological type of object.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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