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The interplay of dense gas and stars in M33

Published online by Cambridge University Press:  21 October 2010

Carsten Kramer
Affiliation:
Instituto Radioastronomia Milimetrica (IRAM), Av. Divina Pastora 7, E-18012 Granada, Spain email: kramer@iram.es
Christof Buchbender
Affiliation:
Instituto Radioastronomia Milimetrica (IRAM), Av. Divina Pastora 7, E-18012 Granada, Spain email: kramer@iram.es
Guillermo Quintana-Lacaci
Affiliation:
Instituto Radioastronomia Milimetrica (IRAM), Av. Divina Pastora 7, E-18012 Granada, Spain email: kramer@iram.es
Jonathan Braine
Affiliation:
Observatoire Bordeaux, LAB - UMR 5804, 2, rue de l'Observatoire, BP 89 -33271 Floirac Cedex - France
Pierre Gratier
Affiliation:
Observatoire Bordeaux, LAB - UMR 5804, 2, rue de l'Observatoire, BP 89 -33271 Floirac Cedex - France
Erik Rosolowsky
Affiliation:
University of British Columbia, 3333 University Way, Kelowna, BC V1V 1V7, Canada
Corresponding
E-mail address:
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Abstract

We are studying the interplay of star formation and its ’fuel’, the molecular gas (diffuse and dense) at selected positions along the major axis of M33. We have observed the ground-state transitions of HCN, HCO+, and 13CO using the IRAM 30m telescope. These data will complement existing CO, HI, Spitzer, and radio continuum maps. Furthermore, these data will be complemented by far-infrared maps of [CII], H2O, [OI], [NII], and the dust continuum taken with Herschel in the open time key project HERM33ES.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

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