[CII] in M33 major axis (HERM33ES)

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We study the photoelectric heating as an approximation of the [CII]/TIR ratio, the correlation between [CII] and other data presented and use [CII] and CO(J=1-0) (calculated through CO (J=2-1)) to study the characteristics of photodissociation regions (PDRs) in the major axis of M33. In addition, we will continue a study from several authors (Stacey et al. 2010, Hailey-Dunsheath et al. 2010, Gracia-Carpio et al. 2011) who have represented galactic and extragalactic studies of [CII] and CO (J=1-0) trying to find common behaviors in different kinds of objects. This work will be followed by studies of specific M33 major axis regions in small-scale, using spectroscopic [CII] data obtained with Herschel/HIFI.
In this work we use ISO/LWS [CII] observations along M33 major axis to make a large-scale study of the PDR and the photoelectric heating in the regions observed. Supplementing these data, we also use data from HERM33ES Herschel Key Project from FIR continuum (Herschel SPIRE, PACS and Spitzer MIPS), CO(J=2-1) (IRAM 30m), HI (VLA) and Halpha (Burrel-Shmidt).

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