activity
20102022
most citedUnveiling the gas and dust disk structure in HD 163296 using ALMA observations

194 citations · 1.3k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2022★ 15 cited

In-depth direct imaging and spectroscopic characterization of the young Solar System analog HD 95086

C. Desgrange, G. Chauvin, V. Christiaens +48

Context. HD 95086 is a young nearby Solar System analog hosting a giant exoplanet orbiting at 57 au from the star between an inner and outer debris belt. The existence of additiona…

astro-ph.EP2021★ 11 cited

The protoplanetary disc around HD 169142: circumstellar or circumbinary?

P. P. Poblete, N. Cuello, S. Pérez +12

Stellar binaries represent a substantial fraction of stellar systems, especially among young stellar objects. Accordingly, binaries play an important role in setting the architectu…

astro-ph.EP2021★ 15 cited

Revealing asymmetrical dust distribution in the inner regions of HD 141569

Garima Singh, Trisha Bhowmik, Anthony Boccaletti +42

We obtained polarimetric differential imaging of a gas-rich debris disk around HD 141569A with SPHERE in the H-band to compare the scattering properties of the innermost ring at 44…

astro-ph.SR2021★ 12 cited

Atomic line radiative transfer with MCFOST I. Code description and benchmarking

B. Tessore, C. Pinte, J. Bouvier +1

Aims. We present MCFOST-art, a new non-local thermodynamic equilibrium radiative transfer solver for multilevel atomic systems. The code is embedded in the 3D radiative transfer co…

astro-ph.SR2020★ 51 cited

FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5

E. Bianchi, C. J. Chandler, C. Ceccarelli +63

The study of hot corinos in Solar-like protostars has been so far mostly limited to the Class 0 phase, hampering our understanding of their origin and evolution. In addition, recen…

astro-ph.SR2019★ 41 cited

ALMA study of the HD 100453 AB system and the tidal interaction of the companion with the disk

G. van der Plas, F. Ménard, J. -F. Gonzalez +6

Context: The complex system HD 100453 AB with a ring-like circumprimary disk and two spiral arms, one of which is pointing to the secondary, is a good laboratory to test spiral for…

astro-ph.SR2016★ 3 cited

Radial decoupling of small and large dust grains in the transitional disk RX J1615.3-3255

Robin Kooistra, Inga Kamp, Misato Fukagawa +56

We present H-band (1.6 μm) scattered light observations of the transitional disk RX J1615.3-3255, located in the ~1 Myr old Lupus association. From a polarized intensity image, tak…

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.EP2015★ 50 cited

Probing the Final Stages of Protoplanetary Disk Evolution with ALMA

A. Hardy, C. Caceres, M. R. Schreiber +5

The evolution of a circumstellar disk from its gas-rich protoplanetary stage to its gas-poor debris stage is not understood well. It is apparent that disk clearing progresses from…

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.EP2014★ 94 cited

CO gas inside the protoplanetary disk cavity in HD 142527: disk structure from ALMA

Sebastian Perez, S. Casassus, F. Ménard +6

Inner cavities and annular gaps in circumstellar disks are possible signposts of giant planet formation. The young star HD 142527 hosts a massive protoplanetary disk with a large c…

astro-ph.SR2014★ 53 cited

A CO survey in planet-forming disks: characterizing the gas content in the epoch of planet formation

A. S. Hales, I. De Gregorio-Monsalvo, B. Montesinos +13

We carried out a 12CO(3-2) survey of 52 southern stars with a wide range of IR excesses (LIR/L*) using the single dish telescopes APEX and ASTE. The main aims were (1) to character…

astro-ph.SR2014★ 59 cited

Constraining the structure of the transition disk HD 135344B (SAO 206462) by simultaneous modeling of multiwavelength gas and dust observations

A. Carmona, C. Pinte, W. F. Thi +14

HD 135344B is an accreting (pre-) transition disk that displays the emission of warm CO extending tens of AU inside its 30 AU dust cavity. We used the dust radiative transfer code…

astro-ph.SR2014★ 86 cited

Gas and dust in the Beta Pictoris Moving Group as seen by the Herschel Space Observatory

P. Riviere-Marichalar, D. Barrado, B. Montesinos +11

Context. Debris discs are thought to be formed through the collisional grinding of planetesimals, and can be considered as the outcome of planet formation. Understanding the proper…

astro-ph.SR2014★ 16 cited

[OI] disk emission in the Taurus star forming region

G. Aresu, I. Kamp, R. Meijerink +8

The structure of protoplanetary disks is thought to be linked to the temperature and chemistry of their dust and gas. Whether the disk is flat or flaring depends on the amount of r…

astro-ph.GA2013★ 79 cited

Herschel/PACS Survey of protoplanetary disks in Taurus/Auriga -- Observations of [OI] and [CII], and far infrared continuum

Christian D. Howard, Göran Sandell, William D. Vacca +17

The Herschel Space Observatory was used to observe ~ 120 pre-main-sequence stars in Taurus as part of the GASPS Open Time Key project. PACS was used to measure the continuum as wel…

astro-ph.SR2013★ 194 cited

Unveiling the gas and dust disk structure in HD 163296 using ALMA observations

I. de Gregorio-Monsalvo, F. Ménard, W. Dent +20

Aims: The aim of this work is to study the structure of the protoplanetary disk surrounding the Herbig Ae star HD 163296. Methods: We have used high-resolution and high-sensitivity…

astro-ph.SR2013★ 45 cited

Gas and dust in the TW Hydrae Association as seen by the Herschel Space Observatory

P. Riviere-Marichalar, C. Pinte, D. Barrado +15

Context. Circumstellar discs are the places where planets form, therefore knowledge of their evolution is crucial for our understanding of planet formation. The Herschel Space Obse…

astro-ph.SR2012★ 52 cited

HD 172555: detection of 63 microns [OI] emission in a debris disc

P. Riviere-Marichalar, D. Barrado, J. -C. Augereau +14

Context. HD 172555 is a young A7 star belonging to the Beta Pictoris Moving Group that harbours a debris disc. The Spitzer IRS spectrum of the source showed mid-IR features such as…

astro-ph.SR2012★ 91 cited

The dynamically disrupted gap in HD 142527

S. Casassus, S. Perez M., A. Jordán +5

The vestiges of planet formation have been observed in debris disks harboring young and massive gaseous giants. The process of giant planet formation is terminated by the dissipati…

astro-ph.SR2011★ 83 cited

Gas modelling in the disc of HD 163296

I. Tilling, P. Woitke, G. Meeus +19

We present detailed model fits to observations of the disc around the Herbig Ae star HD 163296. This well-studied object has an age of ~ 4 Myr, with evidence of a circumstellar dis…

astro-ph.SR2011★ 71 cited

The Late Stages of Protoplanetary Disk Evolution: A Millimeter Survey of Upper Scorpius

Geoffrey S. Mathews, Jonathan P. Williams, Francois Ménard +3

We present deep 1.2 millimeter photometry of 37 stars in the young (5 Myr) Upper Scorpius OB association, sensitive to ~4 x 10^-3 Mjup of cool millimeter dust. Disks around four lo…

astro-ph.EP2011★ 81 cited

The unusual protoplanetary disk around the T Tauri star ET Cha

P. Woitke, B. Riaz, G. Duchene +15

We present new continuum and line observations, along with modelling, of the faint (6-8) Myr old T Tauri star ET Cha belonging to the eta Chamaeleontis cluster. We have acquired HE…

astro-ph.SR2010★ 3 cited

Gas in Protoplanetary Discs (GASPS) 1. First results

G. S. Mathews, W. R. F. Dent, J. P. Williams +50

Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the…