activity
20122017
most citedCan dead zones create structures like a transition disk?

134 citations · 674 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2017★ 75 cited

Inferring giant planets from ALMA millimeter continuum and line observations in (transition) disks

Stefano Facchini, Paola Pinilla, Ewine F. van Dishoeck +1

Potential signatures of proto-planets embedded in their natal protoplanetary disk are radial gaps or cavities in the continuum emission in the IR-mm wavelength range. ALMA observat…

astro-ph.IM2017★ 81 cited

Adapting astronomical source detection software to help detect animals in thermal images obtained by unmanned aerial systems

S. N. Longmore, R. P. Collins, S. Pfeifer +7

In this paper we describe an unmanned aerial system equipped with a thermal-infrared camera and software pipeline that we have developed to monitor animal populations for conservat…

astro-ph.EP2016★ 134 cited

Can dead zones create structures like a transition disk?

Paola Pinilla, Mario Flock, Maria de Juan Ovelar +1

[Abridged] Regions of low ionisation where the activity of the magneto-rotational instability is suppressed, the so-called dead zones, have been suggested to explain gaps and asymm…

astro-ph.SR2014★ 17 cited

Surprising detection of an equatorial dust lane on the AGB star IRC+10216

S. V. Jeffers, M. Min, L. B. F. M. Waters +6

Understanding the formation of planetary nebulae remains elusive because in the preceding asymtotic giant branch (AGB) phase these stars are heavily enshrouded in an optically thic…

astro-ph.EP2014★ 95 cited

Gas and dust structures in protoplanetary disks hosting multiple planets

P. Pinilla, M. de Juan Ovelar, S. Ataiee +4

Transition disks have dust-depleted inner regions and may represent an intermediate step of an on-going disk dispersal process, where planet formation is probably in progress. Rece…

astro-ph.EP2014★ 83 cited

Protoplanetary disc evolution affected by star-disc interactions in young stellar clusters

Giovanni P. Rosotti, James E. Dale, Maria de Juan Ovelar +4

Most stars form in a clustered environment. Therefore, it is important to assess how this environment influences the evolution of protoplanetary discs around young stars. In turn,…

astro-ph.IM2013★ 29 cited

Instrumental polarisation at the Nasmyth focus of the E-ELT

M. de Juan Ovelar, F. Snik, C. U. Keller +1

The ~39-m European Extremely Large Telescope (E-ELT) will be the largest telescope ever built. This makes it particularly suitable for sensitive polarimetric observations, as polar…

astro-ph.EP2013★ 115 cited

Imaging diagnostics for transitional discs

M. de Juan Ovelar, M. Min, C. Dominik +4

Transitional discs are a special type of protoplanetary discs where planet formation is thought to be taking place. These objects feature characteristic inner cavities and/or gaps…

astro-ph.IM2012★ 21 cited

The Extreme Polarimeter: Design, Performance, First Results & Upgrades

M. Rodenhuis, H. Canovas, S. V. Jeffers +4

Well over 700 exoplanets have been detected to date. Only a handful of these have been observed directly. Direct observation is extremely challenging due to the small separation an…

astro-ph.IM2012★ 6 cited

M&m's: An error budget and performance simulator code for polarimetric systems

Maria de Juan Ovelar, Frans Snik, Christoph U. Keller

Although different approaches to model a polarimeter's accuracy have been described before, a complete error budgeting tool for polarimetric systems has not been yet developed. Bas…

astro-ph.SR2012★ 18 cited

Direct imaging of a massive dust cloud around R Coronae Borealis

S. V. Jeffers, M. Min, L. B. F. M. Waters +5

We present recent polarimetric images of the highly variable star R CrB using ExPo and archival WFPC2 images from the HST. We observed R CrB during its current dramatic minimum whe…