most citedThe Herschel-SPIRE instrument and its in-flight performance

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astro-ph.SR2024

MINDS. JWST-MIRI Observations of a Spatially Resolved Atomic Jet and Polychromatic Molecular Wind Toward SY Cha

Kamber R. Schwarz, Matthias Samland, Göran Olofsson +21

The removal of angular momentum from protostellar systems drives accretion onto the central star and may drive the dispersal of the protoplanetary disk. Winds and jets can contribu…

astro-ph.SR2010★ 38 cited

Silicon in the dust formation zone of IRC +10216 as observed with PACS and SPIRE on board Herschel

L. Decin, J. Cernicharo, M. J. Barlow +36

The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which…

astro-ph.SR2010★ 35 cited

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…

astro-ph.SR2010★ 40 cited

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…

astro-ph.SR2010★ 53 cited

Resolving the cold debris disc around a planet-hosting star: PACS photometric imaging observations of q1 Eri (HD10647, HR506)

R. Liseau, C. Eiroa, D. Fedele +32

About two dozen exo-solar debris systems have been spatially resolved. These debris discs commonly display a variety of structural features such as clumps, rings, belts, eccentric…

astro-ph.SR2010★ 42 cited

Herschel PACS and SPIRE imaging of CW Leo

D. Ladjal, M. J. Barlow, M. A. T. Groenewegen +25

Herschel PACS and SPIRE images have been obtained over a 30'x30' area around the well-known carbon star CW Leo (IRC +10 216). An extended structure is found in an incomplete arc of…