The Fate of Star Formation in Chamaeleon I and III
Language
en
Communication dans un congrès
This item was published in
Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster #1K007, 2013, Heidelberg.
English Abstract
The nearby Chamaeleon molecular cloud complex is an excellent laboratory for studying the process of low-mass star formation because it consists of three clouds with very different properties. Chamaeleon III does not show ...Read more >
The nearby Chamaeleon molecular cloud complex is an excellent laboratory for studying the process of low-mass star formation because it consists of three clouds with very different properties. Chamaeleon III does not show any sign of star formation, while star formation has been very active in Chamaeleon I and may already be finishing. We will present the results of an unbiased continuum survey for starless and protostellar cores performed toward both clouds with the Large APEX Bolometer Array (LABOCA) at 870 microns. We will discuss the dynamical state and fate of the starless cores detected in both clouds.Read less <
Origin
Hal imported