activity
20032023
most cited[O I] 6300A emission in Herbig Ae/Be systems: signature of Keplerian rotation

183 citations · 2.5k across the 43 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.EP2012★ 60 cited

Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt

B. L. de Vries, B. Acke, J. A. D. L. Blommaert +20

Some planetary systems harbour debris disks containing planetesimals such as asteroids and comets. Collisions between such bodies produce small dust particles, the spectral feature…

astro-ph.SR2012★ 65 cited

The orbits of subdwarf B + main-sequence binaries. I: The sdB+G0 system PG 1104+243

J. Vos, R. H. Östensen, P. Degroote +18

The predicted orbital period histogram of an sdB population is bimodal with a peak at short (< 10 days) and long (> 250 days) periods. Observationally, there are many short-period…

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.CO2012★ 2 cited

A background galaxy in the field of the beta Pic debris disk

S. Regibo, B. Vandenbussche, C. Waelkens +9

Herschel images in six photometric bands show the thermal emission of the debris disk surrounding beta Pic. In the three PACS bands at 70 micron, 100 micron and 160 micron and in t…

astro-ph.SR2012★ 39 cited

The Spitzer Spectroscopic Survey of S-type Stars

K. Smolders, P. Neyskens, J. A. D. L. Blommaert +28

S-type AGB stars are thought to be in the transitional phase between M-type and C-type AGB stars. Because of their peculiar chemical composition, one may expect a strong influence…

astro-ph.SR2012★ 19 cited

The dynamic atmospheres of Mira stars: comparing the CODEX models to PTI time series of TU And

M. Hillen, T. Verhoelst, P. Degroote +2

Our comprehension of stellar evolution on the AGB still faces many difficulties. To improve on this, a quantified understanding of large-amplitude pulsator atmospheres and interpre…