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20192026
most citedThe Ophiuchus DIsc Survey Employing ALMA (ODISEA)-III: the evolution of substructures in massive discs at 3-5 au resolution

129 citations · 250 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2023

Radio-continuum decrements associated to shadowing from the central warp in transition disc DoAr44

Carla Arce-Tord, Simon Casassus, William R. F. Dent +8

Warps have often been used to explain disc properties, but well characterised examples are important due to their role in disc evolution. Scattered light images of discs with centr…

astro-ph.EP2023★ 1 cited

Azimuthal temperature variations in ISO-Oph2 from multi-frequency ALMA observations

Simon Casassus, Lucas Cieza, Miguel Cárcamo +10

Environmental effects, such as stellar fly-bys and external irradiation, are thought to affect the evolution of protoplanetary disks in clustered star formation. Previous ALMA imag…

astro-ph.EP2021★ 14 cited

High-resolution ALMA observations of V4046Sgr: a circumbinary disc with a thin ring

Rafael Martinez-Brunner, Simon Casassus, Sebastián Pérez +8

The nearby V4046 Sgr spectroscopic binary hosts a gas-rich disc known for its wide cavity and dusty ring. We present high resolution (20 mas or 1.4 au) ALMA observations of t…

astro-ph.EP2021★ 55 cited

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.EP2020★ 129 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★ 16 cited

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…