activity
20032021
most citedThe AGB superwind speed at low metallicity

132 citations · 473 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2021

Will the Mars Helicopter Induce Local Martian Atmospheric Breakdown?

W. M. Farrell, J. L. McLain, J. R. Marshall +1

Any rotorcraft on Mars will fly in a low pressure and dusty environment. It is well known that helicopters on Earth become highly-charged due, in part, to triboelectric effects whe…

astro-ph.IM2017★ 85 cited

OSIRIS-REx Contamination Control Strategy and Implementation

J. P. Dworkin, L. A. Adelman, T. Ajluni +59

OSIRIS-REx will return pristine samples of carbonaceous asteroid Bennu. This article describes how pristine was defined based on expectations of Bennu and on a realistic understand…

astro-ph.EP2014★ 17 cited

The Design Reference Asteroid for the OSIRIS-REx Mission Target (101955) Bennu

Carl W. Hergenrother, Maria Antonietta Barucci, Olivier Barnouin +23

The Design Reference Asteroid (DRA) is a compilation of all that is known about the OSIRIS-REx mission target, asteroid (101955) Bennu. It contains our best knowledge of the proper…

astro-ph2005★ 56 cited

Very Large Telescope three micron spectra of dust-enshrouded red giants in the Large Magellanic Cloud

Jacco Th. van Loon, Jonathan R. Marshall, Martin Cohen +4

We present ESO/VLT spectra in the 2.9--4.1 micron range for a large sample of infrared stars in the Large Magellanic Cloud (LMC), selected on the basis of MSX and 2MASS colours to…

astro-ph2005★ 83 cited

Dust-enshrouded giants in clusters in the Magellanic Clouds

Jacco Th. van Loon, Jonathan R. Marshall, Albert A. Zijlstra

We present the results of an investigation of post-Main Sequence mass loss from stars in clusters in the Magellanic Clouds, based around an imaging survey in the L'-band (3.8 micro…

astro-ph2005★ 73 cited

Three-micron spectra of AGB stars and supergiants in nearby galaxies

M. Matsuura, A. A. Zijlstra, J. Th. van Loon +7

The dependence of stellar molecular bands on the metallicity is studied using infrared L-band spectra of AGB stars (both carbon-rich and oxygen-rich) and M-type supergiants in the…