The goal of the "Evolution of interstellar dust" guaranteed time key project
(PI: A. Abergel & A. Zavagno) is to explore with Herschel the far-infrared
(FIR) to submillimeter (submm) emission properties of dust particles in a wide
range of regions within our Galaxy, from very diffuse clouds to sites of star
formation and proto-stars. Photometric data taken with SPIRE and PACS are
complemented with spectroscopy using the FTS of SPIRE and PACS to derive the
physical conditions of the gas from the lines of [CI], the high-level rotational
lines of CO, and the major cooling lines of [CII] and [OI].
If you use SAG-4 data, please cite both the journal article Abergel et al.
(2010) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA77.
Jump to documentation.
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