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20112021
most citedObservations of gas flows inside a protoplanetary gap

386 citations · 2.5k across the 36 of their papers we have counts for

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astro-ph.SR2021★ 22 cited

Probing protoplanetary disk evolution in the Chamaeleon II region

M. Villenave, F. Menard, W. R. F. Dent +13

Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understanding of planet formation. Constraints on both dust and gas are needed to determin…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.SR2020★ 46 cited

The Ophiuchus DIsc Survey Employing ALMA (ODISEA). II. The effect of stellar multiplicity on disc properties

Alice Zurlo, Lucas A. Cieza, Sebastián Pérez +9

We present Adaptive Optics (AO) near infrared (NIR) observations using VLT/NACO and Keck/NIRC2 of ODISEA targets. ODISEA is an ALMA survey of the entire population of circumstellar…

astro-ph.SR2020★ 45 cited

Exocomets: A spectroscopic survey

I. Rebollido, C. Eiroa, B. Montesinos +18

While exoplanets are now routinely detected, the detection of small bodies in extrasolar systems remains challenging. Since the discovery of sporadic events interpreted as exocomet…

astro-ph.SR2018★ 54 cited

Alma Survey Of Circumstellar Disks In The Young Stellar Cluster IC 348

D. Ruíz-Rodríguez, L. A. Cieza, J. P. Williams +7

We present a 1.3 mm continuum survey of the young (2-3 Myr) stellar cluster IC 348, which lies at a distance of 310 pc, and is dominated by low-mass stars (M 0.1-0…

astro-ph.SR2018★ 46 cited

Resolving faint structures in the debris disk around TWA7

J. Olofsson, R. G. van Holstein, A. Boccaletti +51

Debris disks are the intrinsic by-products of the star and planet formation processes. Most likely due to instrumental limitations and their natural faintness, little is known abou…

astro-ph.SR2018★ 38 cited

The co-existence of hot and cold gas in debris discs

I. Rebollido, C. Eiroa, B. Montesinos +19

Debris discs have often been described as gas-poor discs as the gas-to-dust ratio is expected to be considerably lower than in primordial,protoplanetary discs. However, recent obse…

astro-ph.SR2017★ 29 cited

The ALMA Early Science View of FUor/EXor objects. IV. Misaligned Outflows in the Complex Star-forming Environment of V1647 Ori and McNeil's Nebula

David A. Principe, Lucas Cieza, Antonio Hales +9

We present Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of the star-forming environment surrounding V1647 Ori, an outbursting FUor/EXor pre-MS star. Dust conti…

astro-ph.SR2017★ 44 cited

A 80 au cavity in the disk around HD 34282

G. van der Plas, F. Menard, H. Canovas +5

Context: Large cavities in disks are important testing grounds for the mechanisms proposed to drive disk evolution and dispersion, such as dynamical clearing by planets and photo-e…

astro-ph.SR2016★ 36 cited

The ALMA Early Science View of FUor/EXor objects. II. The Very Wide Outflow Driven by HBC 494

D. Ruíz-Rodríguez, L. A. Cieza, J. P. Williams +10

We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle-2 observations of the HBC 494 molecular outflow and envelope. HBC 494 is an FU Ori-like object embedded in the…

astro-ph.SR2016★ 38 cited

The ALMA Early Science view of FUor/EXor objects. I. Through the looking-glass of V2775 Ori

Alice Zurlo, Lucas A. Cieza, Jonathan P. Williams +11

As part of an ALMA survey to study the origin of episodic accretion in young eruptive variables, we have observed the circumstellar environment of the star V2775 Ori. This object i…

astro-ph.SR2016★ 102 cited

A cavity and further radial substructures in the disk around HD~97048

G. van der Plas, C. M. Wright, F. Ménard +9

Context: Gaps, cavities and rings in circumstellar disks are signposts of disk evolution and planet-disk interactions. We follow the recent suggestion that Herbig Ae/Be disks with…

astro-ph.SR2016★ 234 cited

Imaging the water-snow line during a protostellar outburst

Lucas A. Cieza, Simon Casassus, John Tobin +13

A snow-line is the region of a protoplanetary disk at which a major volatile, such as water or carbon monoxide, reaches its condensation temperature. Snow-lines play a crucial role…

astro-ph.SR2016★ 49 cited

A ring-like concentration of mm-sized particles in Sz 91

H. Canovas, C. Caceres, M. R. Schreiber +4

Models of planet formation and disc evolution predict a variety of observables in the dust structure of protoplanetary discs. Here we present Atacama Large Millimeter/submillimeter…

astro-ph.SR2016★ 108 cited

Azimuthal asymmetries in the debris disk around HD61005

J. Olofsson, M. Samland, H. Avenhaus +30

Debris disks offer valuable insights into the latest stages of circumstellar disk evolution, and can possibly help us to trace the outcomes of planetary formation processes. In the…

astro-ph.SR2015★ 81 cited

Non-azimuthal linear polarization in protoplanetary disks

H. Canovas, F. Ménard, J. de Boer +3

Several studies discussing imaging polarimetry observations of protoplanetary disks use the so-called radial Stokes parameters Q_phi and U_phi to discuss the results. This approach…

astro-ph.SR2015★ 25 cited

The inner environment of Z~CMa: High-Contrast Imaging Polarimetry with NaCo

H. Canovas, S. Perez, C. Dougados +7

Context. Z\,CMa is a binary composed of an embedded Herbig Be and an FU Ori class star separated by au. Observational evidence indicate a complex environment in which eac…

astro-ph.SR2015★ 34 cited

Gas inside the 97 au cavity around the transition disk Sz\,91

H. Canovas, M. R. Schreiber, C. Cáceres +9

We present ALMA (Cycle 0) band-6 and band-3 observations of the transition disk Sz\,91. The disk inclination and position angle are determined to be $i=49.5\degr\pm3.5\degr$ and $\…

astro-ph.SR2013★ 87 cited

Near-Infrared Imaging Polarimetry of HD142527

H. Canovas, F. Menard, A. Hales +5

HD 142527 is a pre-transition disk with strong evidence for on-going planet formation. Recent observations show a disrupted disk with spiral arms, a dust-depleted inner cavity and…

astro-ph.SR2013★ 24 cited

The color dependent morphology of the post-AGB star HD161796

M. Min, S. V. Jeffers, H. Canovas +3

Context. Many protoplanetary nebulae show strong asymmetries in their surrounding shell, pointing to asymmetries during the mass loss phase. Questions concerning the origin and the…