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The dust masses of powerful radio galaxies: clues to the triggering of their activity
C. Tadhunter, D. Dicken, R. Morganti +4
We use deep Herschel Space Observatory observations of a 90% complete sample of 32 intermediate-redshift 2Jy radio galaxies (0.05 < z < 0.7) to estimate the dust masses of their ho…
Class 0 Protostars in the Perseus Molecular Cloud: A Correlation Between the Youngest Protostars and the Dense Gas Distribution
S. I. Sadavoy, J. Di Francesco, Ph. Andre +18
We use PACS and SPIRE continuum data at 160 um, 250 um, 350 um, and 500 um from the Herschel Gould Belt Survey to sample seven clumps in Perseus: B1, B1-E, B5, IC348, L1448, L1455,…
Herschel's view of the large-scale structure in the Chamaeleon dark clouds
C. Alves de Oliveira, N. Schneider, B. Merín +17
The Chamaeleon molecular cloud complex is one of the nearest star-forming sites encompassing three molecular clouds with a different star-formation history, from quiescent (Cha III…
A Herschel and BIMA study of the sequential star formation near the W48A HII region
K. L. J. Rygl, S. Goedhart, D. Polychroni +22
We present the results of Herschel HOBYS photometric mapping combined with BIMA observations and additional archival data, and perform an in-depth study of the evolutionary phases…
Properties of Starless and Prestellar Cores in Taurus Revealed by Herschel SPIRE/PACS Imaging
K. A. Marsh, M. J. Griffin, P. Palmeirim +18
The density and temperature structures of dense cores in the L1495 cloud of the Taurus star-forming region are investigated using Herschel SPIRE and PACS images in the 70 m, 160…
SPIRE Map-Making Test Report
C. Kevin Xu, Hacheme Ayasso, Alexandre Beelen +7
The photometer section of SPIRE is one of the key instruments on board of Herschel. Its legacy depends very much on how well the scanmap observations that it carried out during the…