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20102025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 3.8k across the 23 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2023

Oxygen abundance of gamma Vel from [O III] 88um Herschel/PACS spectroscopy

Paul A Crowther, M J Barlow, P Royer +4

We present Herschel PACS spectroscopy of the [O III] 88.4um fine-structure line in the nearby WC8+O binary system gamma Vel to determine its oxygen abundance. The critical density…

astro-ph.SR2018★ 7 cited

PACS and SPIRE range spectroscopy of cool, evolved stars

Dries Nicolaes, M. A. T. Groenewegen, P. Royer +3

Context: At the end of their lives AGB stars are prolific producers of dust and gas. The details of this mass-loss process are still not understood very well. Herschel PACS and SPI…

astro-ph.SR2016★ 5 cited

Evolutionary status of the Of?p star HD148937 and of its surrounding nebula NGC6164/5

L. Mahy, D. Hutsemékers, Y. Nazé +3

Aims. The magnetic star HD148937 is the only Galactic Of?p star surrounded by a nebula. The structure of this nebula is particularly complex and is composed, from the center out ou…

astro-ph.SR2016★ 13 cited

Tracing back the evolution of the candidate LBV HD168625

L. Mahy, D. Hutsemékers, P. Royer +1

Aims. We obtained Herschel/PACS imaging and spectroscopic observations of the nebula surrounding the candidate LBV HD168625. By combining these data with optical spectra of the sta…

astro-ph.SR2016★ 11 cited

Herschel observations of the nebula M1-67 around the Wolf-Rayet star WR 124

C. Vamvatira-Nakou, D. Hutsemekers, P. Royer +3

Infrared Herschel imaging and spectroscopic observations of the nebula M1-67 around the Wolf-Rayet star WR 124 have been obtained along with optical imaging observations. The infra…

astro-ph.SR2014★ 18 cited

Herschel spectral-mapping of the Helix Nebula (NGC 7293): Extended CO photodissociation and OH+ emission

M. Etxaluze, J. Cernicharo, J. R. Goicoechea +13

The Helix Nebula (NGC 7293) is the closest planetary nebulae. Therefore, it is an ideal template for photochemical studies at small spatial scales in planetary nebulae. We aim to s…