most citedThe evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

446 citations · 637 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016138 cited

DustPedia - A Definitive Study of Cosmic Dust in the Local Universe

J. I. Davies, M. Baes, S. Bianchi +20

The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…

astro-ph.GA201632 cited

The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus

S. Bianchi, C. Giovanardi, M. W. L. Smith +22

We study the correlation between far-infared/submm dust emission and atomic gas column density in order to derive the properties of the high Galactic latitude, low density, Milky W…

astro-ph.GA2014

The physical and compositional properties of dust: what do we really know?

Ant Jones

Many things in current interstellar dust studies are taken as well understood givens by much of the community. For example, it is widely held that interstellar dust is made up of o…

astro-ph.GA2014446 cited

The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

A. P. Jones, L. Fanciullo, M. Koehler +4

Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption- induced processing, are likely at the heart of th…

astro-ph.GA201420 cited

Heteroatom-doped hydrogenated amorphous carbons, a-C:H:X 'Volatile' silicon, sulphur and nitrogen depletion, blue photoluminescence, diffuse interstellar bands and ferro-magnetic carbon grain connections (Research Note)

A. P. Jones

Context. Hydrogenated amorphous carbons, a-C:H, can incorporate a variety of heteroatoms, which can lead to interesting effects. Aims. To investigate the doping of interstellar a-C…

astro-ph.GA20141 cited

Interstellar and circumstellar fullerenes

J. Bernard-Salas, J. Cami, A. P. Jones +6

Fullerenes are a particularly stable class of carbon molecules in the shape of a hollow sphere or ellipsoid that might be formed in the outflows of carbon stars. Once injected into…