activity
20192021
most citedThe Ophiuchus DIsc Survey Employing ALMA (ODISEA)-III: the evolution of substructures in massive discs at 3-5 au resolution

129 citations · 129 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2021

A dusty filament and turbulent CO spirals in HD135344B-SAO206462

Simon Casassus, Valentin Christiaens, Miguel Carcamo +16

Planet-disc interactions build up local pressure maxima that may halt the radial drift of protoplanetary dust, and pile it up in rings and crescents. ALMA observations of the HD135…

astro-ph.EP2020129 cited

The Ophiuchus DIsc Survey Employing ALMA (ODISEA)-III: the evolution of substructures in massive discs at 3-5 au resolution

Lucas A. Cieza, Camilo González-Ruilova, Antonio S. Hales +15

We present 1.3 mm continuum ALMA long-baseline observations at 3-5 au resolution of 10 of the brightest discs from the Ophiuchus DIsc Survey Employing ALMA (ODISEA) project. We ide…

astro-ph.EP2020

A Tale of Two Transition Disks: ALMA long-baseline observations of ISO-Oph 2 reveal two closely packed non-axisymmetric rings and a 2 au cavity

Camilo González-Ruilova, Lucas A. Cieza, Antonio S. Hales +12

ISO-Oph 2 is a wide-separation (240 au) binary system where the primary star harbors a massive (M 40 M) ring-like disk with a dust cavity 50 au in r…

astro-ph.GA2020

Resolved spectral variations of the centimetre-wavelength continuum from the rho Oph W photo-dissociation-region

Simon Casassus, Matias Vidal, Carla Arce-Tord +5

Cm-wavelength radio continuum emission in excess of free-free, synchrotron and Rayleigh-Jeans dust emission (excess microwave emission, EME), and often called `anomalous microwave…

astro-ph.GA2019

Resolved observations at 31 GHz of spinning dust emissivity variations in Oph

Carla Arce-Tord, Matias Vidal, Simon Casassus +9

The Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the Cosmic Background Imager (CBI). Here we present 4.5 arcmin observations wit…