activity
20122017
most citedGaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations

379 citations · 568 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2017★ 33 cited

First millimeter detection of the disk around a young, isolated, planetary-mass object

Amelia Bayo, Viki Joergens, Yao Liu +12

OTS44 is one of only four free-floating planets known to have a disk. We have previously shown that it is the coolest and least massive known free-floating planet (12 M$_{\rm…

astro-ph.EP2016★ 88 cited

Gaps, rings, and non-axisymmetric structures in protoplanetary disks - Emission from large grains

J. P. Ruge, M. Flock, S. Wolf +5

Dust grains with sizes around (sub)mm are expected to couple only weakly to the gas motion in regions beyond 10 au of circumstellar disks. In this work, we investigate the influenc…

astro-ph.EP2015★ 14 cited

Structures in circumbinary disks: Prospects for observability

Jan Philipp Ruge, Sebastian Wolf, Tatiana Demidova +1

During the past decade circumbinary disks have been discovered around various young binary stars. Hydrodynamical calculations indicate that the gravitational interaction between th…

astro-ph.EP2014★ 379 cited

Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations

M. Flock, J. P. Ruge, N. Dzyurkevich +3

Recent observations by the Atacama Large Millimeter/submillimeter Array (ALMA) of disks around young stars revealed distinct asymmetries in the dust continuum emission. In this wor…

astro-ph.EP2014★ 12 cited

Planet-induced disk structures: A comparison between (sub)mm and infrared radiation

Jan Philipp Ruge, Sebastian Wolf, Ana L. Uribe +1

Young giant planets, which are embedded in a circumstellar disk, will significantly perturb the disk density distribution. This effect can potentially be used as an indirect tracer…

astro-ph.SR2012★ 42 cited

Tracing large-scale structures in circumstellar disks with ALMA

Jan Philipp Ruge, Sebastian Wolf, Ana L. Uribe +1

Planets are supposed to form in circumstellar disks. The gravitational potential of a planet perturbs the disk and leads to characteristic structures, i.e. spiral waves and gaps, i…