activity
19992014
most citedHerschel/PACS observations of the 69 band of crystalline olivine around evolved stars

30 citations · 57 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2014★ 30 cited

Herschel/PACS observations of the 69 band of crystalline olivine around evolved stars

J. A. D. L. Blommaert, B. L. de Vries, L. B. F. M. Waters +15

We present 48 Herschel/PACS spectra of evolved stars in the wavelength range of 67-72 m. This wavelength range covers the 69 m band of crystalline olivine ($\text{Mg}_{2-2x}\…

astro-ph.GA2013★ 27 cited

Herschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra

Mikako Matsuura, J. A. Yates, M. J. Barlow +10

We present an analysis of the far-infrared and submillimetre molecular emission line spectrum of the luminous M-supergiant VY CMa, observed with the SPIRE and PACS spectrometers ab…

astro-ph.SR2011

Herschel observations of PNe in the MESS key program

P. A. M. van Hoof, M. J. Barlow, G. C. Van de Steene +10

In this paper we give a progress report on the Herschel imaging and spectroscopic observations of planetary nebulae that are carried out as part of the MESS guaranteed time key pro…

astro-ph.SR2011

A Herschel study of Planetary Nebulae

G. C. Van de Steene, K. M. Exter, P. A. M. van Hoof +5

We present Herschel PACS and SPIRE images of the dust shells around the planetary nebulae NGC 650, NGC 6853, and NGC 6720, as well as images showing the dust temperature in their s…

astro-ph.SR2010

Imaging Planetary Nebulae with Herschel-PACS and SPIRE

P. A. M. van Hoof, K. M. Exter, G. C. Van de Steene +25

In this paper we will discuss the images of Planetary Nebulae that have recently been obtained with PACS and SPIRE on board the Herschel satellite. This comprises results for NGC 6…

astro-ph1999

The central stars of the planetary nebulae NGC 7027 and NGC 6543

D. A. Beintema, P. A. M. van Hoof, F. Lahuis +6

Infrared spectra of NGC 7027 and NGC 6543 ranging from 2.4 to 45 micron were obtained with the Short Wavelength Spectrometer on board the Infrared Space Observatory. A first analys…