High Mass Star Forming Gas in Cygnus X: The Molecular and Spitzer View of the DR21 Region
BONTEMPS, Sylvain
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Observatoire aquitain des sciences de l'univers [OASU]
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Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Observatoire aquitain des sciences de l'univers [OASU]
BONTEMPS, Sylvain
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Observatoire aquitain des sciences de l'univers [OASU]
< Reduce
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Observatoire aquitain des sciences de l'univers [OASU]
Language
en
Communication dans un congrès
This item was published in
The Spitzer Space Telescope: New Views of the Cosmos - ASP Conference Series Volume 357 - 2006, The Spitzer Space Telescope: New Views of the Cosmos - ASP Conference Series Volume 357 - 2006, The Spitzer Space Telescope: New Views of the Cosmos, 2004-11-09, pasadena. 2006, vol. 357, p. 153
English Abstract
n order to study the processes by which rich clusters and high-mass stars form and evolve, we started a large scale molecular line and mm-continuum survey of Cygnus X, one of the richest and most active regions of our ...Read more >
n order to study the processes by which rich clusters and high-mass stars form and evolve, we started a large scale molecular line and mm-continuum survey of Cygnus X, one of the richest and most active regions of our Galaxy. From this ongoing survey, we use molecular line observations (FCRAO, IRAM 30m) to investigate the relationship between molecular gas and the dust as seen in recently published IRAC and MIPS data of the DR21/W75 region.Read less <
Origin
Hal imported