196 citations · 616 across the 8 of their papers we have counts for
8 papers
From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?
Lars Mattsson, Haley L. Gomez, Anja C. Andersen +1
The amount of dust estimated from infrared to sub-millimetre (submm) observations strongly depends on assumptions of different grain sizes, compositions and optical properties. Her…
The β Pictoris disk imaged by Herschel PACS and SPIRE
B. Vandenbussche, B. Sibthorpe, B. Acke +40
We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star β Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 μ…
The Vega Debris Disc: A view from Herschel
B. Sibthorpe, B. Vandenbussche, J. S. Greaves +37
We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 um with full-width half-maximum ang…
Herschel-SPIRE FTS spectroscopy of the carbon-rich objects AFGL 2688, AFGL 618 and NGC 7027
R. Wesson, J. Cernicharo, M. J. Barlow +22
We present far-infrared and submillimetre spectra of three carbon-rich evolved objects, AFGL 2688, AFGL 618 and NGC 7027. The spectra were obtained with the SPIRE Fourier transform…
A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant
M. J. Barlow, O. Krause, B. M. Swinyard +13
Using the 3.5-m Herschel Space Observatory, imaging photometry of Cas A has been obtained in six bands between 70 um and 500 um with the PACS and SPIRE instruments, with angular re…
Mapping the interstellar medium in galaxies with Herschel/SPIRE
S. A. Eales, M. W. L. Smith, C. D. Wilson +57
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…