activity
20162022
most citedMolecular gas in debris disks around young A-type stars

114 citations · 257 across the 9 of their papers we have counts for

collaborators

15 papers

astro-ph.EP20229 cited

High resolution ALMA and HST imaging of CrB: a broad debris disc around a post-main sequence star with low-mass companions

J. B. Lovell, M. C. Wyatt, P. Kalas +6

CrB is a Gyr old K1 sub-giant star, with an eccentric exo-Jupiter at au and a debris disc at tens of au. We present ALMA Band 6 (mm) and HST sca…

astro-ph.SR202120 cited

Characterizing the morphology of the debris disk around the low-mass star GSC~07396-00759

C. Adam, J. Olofsson, R. G. van Holstein +17

Context. Debris disks have commonly been studied around intermediate-mass stars. Their intense radiation fields are believed to efficiently remove the small dust grains that are co…

astro-ph.EP202140 cited

A Occurrence Rate of Debris Discs around F stars in the Pic Moving Group

Nicole Pawellek, Mark Wyatt, Luca Matrà +2

Only 20\% of old field stars have detectable debris discs, leaving open the question of what disc, if any, is present around the remaining 80\%. Young moving groups allow to probe…

astro-ph.SR202013 cited

The big sibling of AU Mic: a cold dust-rich debris disk around CP-72 2713 in the Pic moving group

A. Moór, N. Pawellek, P. Ábrahám +8

Analyzing Spitzer and Herschel archival measurements we identified a debris disk around the young K7/M0 star CP-72 2713. The system belongs to the 24Myr old Pic moving group. O…

astro-ph.EP201918 cited

HD 117214 debris disk: scattered-light images and constraints on the presence of planets

N. Engler, C. Lazzoni, R. Gratton +34

We performed observations of the Sco-Cen F star HD 117214 aiming at a search for planetary companions and the characterization of the debris disk structure. HD 117214 was observed…

astro-ph.SR2019

Dust production in the debris disk around HR 4796 A

J. Olofsson, J. Milli, P. Thébault +21

Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from…