activity
20082021
most citedThermal properties of slowly rotating asteroids: Results from a targeted survey

29 citations · 61 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202120 cited

Outbursts and stellar properties of the classical Be star HD 6226

Noel D. Richardson, Olivier Thizy, Jon E. Bjorkman +58

The bright and understudied classical Be star HD 6226 has exhibited multiple outbursts in the last several years during which the star grew a viscous decretion disk. We analyze 659…

astro-ph.SR20199 cited

Evolution of the disk of pi Aqr: from near-disappearance to a strong maximum

Y. Naze, G. Rauw, J . Guarro Flo +30

Some Be stars display important variability of the strength of the emission lines formed in their disk. This is notably the case of pi Aqr. We present here the recent evolution of…

astro-ph.EP201929 cited

Thermal properties of slowly rotating asteroids: Results from a targeted survey

A. Marciniak, V. Alí-Lagoa, T. G. Müller +51

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface.…

astro-ph.SR20121 cited

High cadence measurement of neutral sodium and potassium absorption during the 2009-2011 eclipse of epsilon Aurigae

R. Leadbeater, C. Buil, T. Garrel +6

The results of a spectroscopic survey of epsilon Aurigae during eclipse using a network of small telescopes are presented. The spectra have a resolution of 0.35 to 0.65Å and cover…

astro-ph20082 cited

The magnetic field of the B3V star 16 Pegasi

H. F. Henrichs, C. Neiner, R. S. Schnerr +8

The Slowly Pulsating B3V star 16 Pegasi was discovered by Hubrig (2006) to be magnetic, based on low-resolution spectropolarimetric observations with FORS1 at the VLT. We have conf…