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The Hi-GAL catalogue of dusty filamentary structures in the Galactic Plane
E. Schisano, S. Molinari, D. Elia +27
The recent data collected by {\it Herschel} have confirmed that interstellar structures with filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to b…
The Forgotten Quadrant Survey. CO and CO (1-0) survey of the Galactic Plane in the range 220°240° -2.5°0°
M. Benedettini, S. Molinari, A. Baldeschi +12
We present the Forgotten Quadrant Survey (FQS), an ESO large project that used the 12m antenna of the Arizona Radio Observatory to map the Galactic Plane in the range 220°240°…
Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey
V. Konyves, Ph. Andre, D. Arzoumanian +15
We present a detailed study of the Orion B clouds (d~400 pc), imaged with the PACS/SPIRE cameras at 70-500 m by the Herschel Gould Belt survey (HGBS). We release new high-res. m…
KFPA Examinations of Young STellar Object Natal Environments (KEYSTONE): Hierarchical Ammonia Structures in Galactic Giant Molecular Clouds
Jared Keown, James Di Francesco, Erik Rosolowsky +23
We present initial results from the K-band focal plane array Examinations of Young STellar Object Natal Environments (KEYSTONE) survey, a large project on the 100-m Green Bank Tele…
How the power spectrum of dust continuum images may hide the presence of a characteristic filament width
Arabindo Roy, Philippe André, Doris Arzoumanian +6
Herschel observations of interstellar clouds support a paradigm for star formation in which filaments play a central role. One of the foundations of this paradigm is the finding, b…