activity
19992023
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 1.4k across the 14 of their papers we have counts for

collaborators

14 papers

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.SR2017★ 44 cited

Carinae's Dusty Homunculus Nebula from Near-Infrared to Submillimeter Wavelengths: Mass, Composition, and Evidence for Fading Opacity

Patrick W. Morris, Theodore R. Gull, D. John Hillier +5

Infrared observations of the dusty, massive Homunculus Nebula around the luminous blue variable Carinae are crucial to characterize the mass-loss history and help constrain the…

astro-ph.SR2016★ 42 cited

Herschel detects oxygen in the beta Pictoris debris disk

A. Brandeker, G. Cataldi, G. Olofsson +28

The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the…

astro-ph.SR2012★ 4 cited

The Outer Wind of gamma Velorum

P. F. Roche, M. D. Colling, M. J. Barlow

Fine-structure mid-infrared emission lines with critical densities in the regime 10^4 to 10^6 cm^-3 can be employed to probe the outflow from Wolf-Rayet stars at radii of \sim 10^1…

astro-ph.SR2012★ 120 cited

Herschel images of Fomalhaut. An extrasolar Kuiper Belt at the height of its dynamical activity

B. Acke, M. Min, C. Dominik +33

Fomalhaut is a young, nearby star that is suspected to harbor an infant planetary system, interspersed with one or more belts of dusty debris. We present far-infrared images obtain…

astro-ph.SR2012★ 42 cited

On the physical structure of IRC+10216. Ground-based and Herschel observations of CO and CCH

E. De Beck, R. Lombaert, M. Agúndez +17

The C-rich AGB star IRC+10216 undergoes strong mass loss, and quasi-periodic density enhancements in the circumstellar matter have been reported. CO is ubiquitous in the CSE, while…