Gas and Dust in M33
Idioma
en
Communication dans un congrès
Este ítem está publicado en
Proceedings of the International Astronomical Union, IAU Symposium 277, Proceedings of the International Astronomical Union, IAU Symposium 277, 2011, Ouagadougou. 2011-12, vol. 277, p. 63-66
Resumen en inglés
We present results from the Herschel and IRAM projects to map M33 in the dust continuum and main emission lines, particularly C[II] and CO. The temperature of the cool dust decreases with distance from the center of M33 ...Leer más >
Palabras clave en inglés
stars: formation
ISM: molecules
dust
extinction
ISM: evolution
ISM: general
ISM: abundances
galaxies: evolution galaxies: formation
Local Group
infrared: ISM