activity
20142019
most citedOld pre-main-sequence Stars: Disc reformation by Bondi-Hoyle accretion

25 citations · 84 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA201919 cited

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 μm data reduction and dust flux density catalogues

Matthew W. L. Smith, Christopher J. R. Clark, Ilse De Looze +33

We present the SCUBA-2 850 component of JINGLE, the new JCMT large survey for dust and gas in nearby galaxies, which with 193 galaxies is the largest targeted survey of nearby…

astro-ph.SR2019

Astro2020 Science White Paper: The fundamentals of outflows from evolved stars

E. De Beck, M. L. Boyer, V. Bujarrabal +16

Models of the chemical evolution of the interstellar medium, galaxies, and the Universe rely on our understanding of the amounts and chemical composition of the material returned b…

astro-ph.SR201916 cited

Resolved imaging of the AR Puppis circumbinary disk

S. Ertel, D. Kamath, M. Hillen +14

Circumbinary disks are common around post-asymptotic giant branch (post-AGB) stars with a stellar companion on orbital time scales of a few 100 to few 1000 days. The presence of a…

astro-ph.IM20165 cited

The Astropy Problem

Demitri Muna, Michael Alexander, Alice Allen +151

The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…

astro-ph.SR201619 cited

XSHOOTER spectroscopy of the enigmatic planetary nebula Lin49 in the Small Magellanic Cloud

Masaaki Otsuka, F. Kemper, M. L. Leal-Ferreira +6

We performed a detailed spectroscopic analysis of the fullerene C60-containing planetary nebula (PN) Lin49 in the Small Magellanic Cloud using XSHOOTER at the ESO VLT and the Spitz…

astro-ph.SR201425 cited

Old pre-main-sequence Stars: Disc reformation by Bondi-Hoyle accretion

P. Scicluna, G. Rosotti, J. E. Dale +1

Young stars show evidence of accretion discs which evolve quickly and disperse with an e-folding time of 3Myr. This is in striking contrast with recent observations that sug…