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Results of the IRAM M33 Large Program
Language
en
Communication dans un congrès
This item was published in
2012, Beijing. 2013-03, vol. 292, p. 135-138
English Abstract
A very sensitive survey of the CO(2-1) emission of the entire disk of the Local Group galaxy M 33 is virtually complete. Hundreds of clouds down to a mass of 10000M&sun; are detected and we show that the cloud mass function ...Read more >
A very sensitive survey of the CO(2-1) emission of the entire disk of the Local Group galaxy M 33 is virtually complete. Hundreds of clouds down to a mass of 10000M&sun; are detected and we show that the cloud mass function (assuming a constant ratio between CO emission and H2 mass) steepens away from the center of M 33. Through comparison with dust emission and cloud Virial masses, we estimate a N(H2)/I CO factor roughly twice Galactic.Read less <
English Keywords
galaxies: individual (M33)
Local Group
galaxies: evolution
galaxies: ISM
ISM: clouds
stars: formation
Origin
Hal imported