activity
20142022
most citedEffect of dust grain porosity on the appearance of protoplanetary disks

41 citations · 118 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA20232 cited

Far-infrared Polarization of the Supernova Remnant Cassiopeia A with SOFIA HAWC+

Jeonghee Rho, Aravind P. Ravi, Le Ngoc Tram +8

We present polarization observations of the young supernova remnant (SNR) Cas A using the High-resolution Airborne Wideband Camera-Plus (HAWC+) instrument onboard the Stratospheric…

astro-ph.GA20228 cited

SOFIA/HAWC+ observations of the Crab Nebula: dust properties from polarised emission

Jérémy Chastenet, Ilse De Looze, Brandon S. Hensley +14

Supernova remnants (SNRs) are well-recognised dust producers, but their net dust production rate remains elusive due to uncertainties in grain properties that propagate into observ…

astro-ph.GA202116 cited

The JCMT BISTRO Survey: Evidence for Pinched Magnetic Fields in Quiescent Filaments of NGC 1333

Yasuo Doi, Kohji Tomisaka, Tetsuo Hasegawa +33

We investigate the internal 3D magnetic structure of dense interstellar filaments within NGC 1333 using polarization data at from the -fields In STar-forming R…

astro-ph.SR201615 cited

The influence of dust grain porosity on the analysis of debris disc observations

Robert Brunngräber, Sebastian Wolf, Florian Kirchschlager +1

Debris discs are often modelled assuming compact dust grains, but more and more evidence for the presence of porous grains is found. We aim at quantifying the systematic errors int…

astro-ph.SR201617 cited

The circumstellar disk of FS Tau B - A self-consistent model based on observations in the mid-infrared with NACO -

Florian Kirchschlager, Sebastian Wolf, David Madlener

Protoplanetary disks are a byproduct of the star formation process. In the dense mid-plane of these disks, planetesimals and planets are expected to form. The first step in planet…

astro-ph.SR201421 cited

Interpreting the extended emission around three nearby debris disc host stars

Jonathan P. Marshall, F. Kirchschlager, S. Ertel +7

Cool debris discs are a relic of the planetesimal formation process around their host star, analogous to the solar system's Edgeworth-Kuiper belt. As such, they can be used as a pr…