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20082026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 7.8k across the 138 of their papers we have counts for

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Showing 2019Show all

17 papers · 1 filter

astro-ph.EP2019★ 24 cited

A dusty benchmark brown dwarf near the ice line of HD 72946

A. -L. Maire, J. -L. Baudino, S. Desidera +12

Context. HD72946 is a bright and nearby solar-type star hosting a low-mass companion at long period (P~16 yr) detected with the radial velocities (RV) method. The companion has a m…

astro-ph.EP2019★ 9 cited

NaCo polarimetric observations of Sz 91 transitional disk: a remarkable case of dust filtering

Karina Maucó, Johan Olofsson, Hector Canovas +10

We present polarized light observations of the transitional disk around Sz 91 acquired with VLT/NaCo at (1.7m) and (2.2m) bands. We resolve the disk and detect pola…

astro-ph.EP2019★ 18 cited

HD 117214 debris disk: scattered-light images and constraints on the presence of planets

N. Engler, C. Lazzoni, R. Gratton +34

We performed observations of the Sco-Cen F star HD 117214 aiming at a search for planetary companions and the characterization of the debris disk structure. HD 117214 was observed…

astro-ph.EP2019★ 8 cited

An unusually large gaseous transit in a debris disc

Daniela P. Iglesias, Johan Olofsson, Amelia Bayo +9

We present the detection of an unusually large transient gas absorption in several ionized species in the debris disc star HD 37306 using high-resolution optical spectra. We have b…

astro-ph.EP2019★ 42 cited

From scattered-light to millimeter emission: A comprehensive view of the Gyr-old system of HD 202628 and its eccentric debris ring

Virginie Faramaz, John Krist, Karl R. Stapelfeldt +13

We present here new observations of the eccentric debris ring surrounding the Gyr-old solar-type star HD 202628: at millimeter wavelengths with ALMA, at far-infrared wavelengths wi…

astro-ph.SR2019★ 25 cited

Dust production in the debris disk around HR 4796 A

J. Olofsson, J. Milli, P. Thébault +21

Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from…

astro-ph.EP2019★ 36 cited

Spatially resolved spectroscopy of the debris disk HD 32297: Further evidence of small dust grains

T. Bhowmik, A. Boccaletti, P. Thébault +14

Spectro-photometry of debris disks in total intensity and polarimetry can provide new insight into the properties of the dust grains therein (size distribution and optical properti…

astro-ph.EP2019★ 11 cited

First resolved observations of a highly asymmetric debris disc around HD 160305 with VLT/SPHERE

Clément Perrot, Philippe Thebault, Anne-Marie Lagrange +36

Context. Direct imaging of debris discs gives important information about their nature, their global morphology, and allows us to identify specific structures possibly in connectio…

astro-ph.EP2019★ 10 cited

A multi-wavelength study of the debris disc around 49 Cet

Nicole Pawellek, Attila Moór, Julien Milli +17

In a multi-wavelength study of thermal emission and scattered light images we analyse the dust properties and structure of the debris disc around the A1-type main sequence star 49~…

astro-ph.EP2019★ 10 cited

ISPY -- NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring

Arianna Musso Barcucci, Ralf Launhardt, Grant M. Kennedy +19

Context. The interaction between low-mass companions and the debris discs they reside in is still not fully understood. A debris disc can evolve due to self-stirring, a process in…

astro-ph.EP2019★ 57 cited

Optical polarized phase function of the HR\,4796A dust ring

J. Milli, N. Engler, H. M. Schmid +24

The scattering properties of the dust originating from debris discs are still poorly known. The analysis of scattered light is however a powerful remote-sensing tool to understand…

astro-ph.EP2019★ 45 cited

Extreme Debris Disk Variability -- Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation

Kate Y. L. Su, Alan P. Jackson, Andras Gaspar +14

The most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between lar…

astro-ph.EP2019★ 44 cited

Hint of curvature in the orbital motion of the exoplanet 51 Eridani b using 3 years of VLT/SPHERE monitoring

A. -L. Maire, L. Rodet, F. Cantalloube +49

Context. The 51 Eridani system harbors a complex architecture with its primary star forming a hierarchical system with the binary GJ 3305AB at a projected separation of 2000 au, a…

astro-ph.SR2019★ 66 cited

Spatial segregation of dust grains in transition disks. SPHERE observations of 2MASS J16083070-3828268 and RXJ1852.3-3700

M. Villenave, M. Benisty, W. R. F. Dent +27

Context. The mechanisms governing the opening of cavities in transition disks are not fully understood. Several processes have been proposed but their occurrence rate is still unkn…

astro-ph.SR2019★ 8 cited

ISPY - the NaCo Imaging Survey for Planets around Young stars: A young companion candidate embedded in the R CrA cloud

G. Cugno, S. P. Quanz, R. Launhardt +13

Within the NaCo-ISPY exoplanet imaging program, we aim at detecting and characterizing the population of low-mass companions at wide separations (10AU), focusing in partic…

astro-ph.EP2019★ 48 cited

On the Ubiquity and Stellar Luminosity Dependence of Exocometary CO Gas: Detection around M Dwarf TWA 7

Luca Matrà, Karin I. Öberg, David J. Wilner +2

Millimeter observations of CO gas in planetesimal belts show a high detection rate around A stars, but few detections for later type stars. We present the first CO detection in a p…

astro-ph.EP2019★ 31 cited

Investigating the presence of two belts in the HD 15115 system

N. Engler, A. Boccaletti, H. M. Schmid +16

We present new observations of the edge-on debris disk around HD 15115 (F star at 48.2 pc) obtained in the near-IR. We search for observational evidence for a second inner planetes…