Herbig Stars: A Quarter Century of Progress

SD Brittain, I Kamp, G Meeus, RD Oudmaijer… - Space Science …, 2023 - Springer
Abstract Herbig Ae/Be stars are young contracting stars on the radiative track in the HR
diagram on their way to the main sequence. These stars provide a valuable link between …

Dusty circumstellar disks

B Zuckerman - Annual Review of Astronomy and Astrophysics, 2001 - annualreviews.org
▪ Abstract Dusty circumstellar disks in orbit around main-sequence stars were discovered in
1983 by the infrared astronomical satellite. It was the first time material that was not another …

Debris disk results from the Gemini Planet Imager Exoplanet Survey's polarimetric imaging campaign

TM Esposito, P Kalas, MP Fitzgerald… - The Astronomical …, 2020 - iopscience.iop.org
We report the results of a∼ 4 yr direct imaging survey of 104 stars to resolve and
characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager …

The JWST early release science program for the direct imaging and spectroscopy of exoplanetary systems

S Hinkley, AL Carter, S Ray, A Skemer… - Publications of the …, 2022 - iopscience.iop.org
The direct characterization of exoplanetary systems with high-contrast imaging is among the
highest priorities for the broader exoplanet community. As large space missions will be …

Two-dimensional radiative transfer in protostellar envelopes. II. An evolutionary sequence

BA Whitney, K Wood, JE Bjorkman… - The Astrophysical …, 2003 - iopscience.iop.org
We present model spectral energy distributions (SEDs), colors, polarization, and images for
an evolutionary sequence of a low-mass protostar from the early collapse stage (Class 0) to …

Resolving the HD 100546 protoplanetary system with the Gemini Planet Imager: evidence for multiple forming, accreting planets

T Currie, R Cloutier, S Brittain, C Grady… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT We report Gemini Planet Imager H-band high-contrast imaging/integral field
spectroscopy and polarimetry of the HD 100546, a 10 Myr old early-type star recently …

Near-infrared scattered light properties of the HR 4796 A dust ring-A measured scattering phase function from 13.6° to 166.6°

J Milli, A Vigan, D Mouillet, AM Lagrange… - Astronomy & …, 2017 - aanda.org
Context. HR 4796 A is surrounded by a debris disc, observed in scattered light as an
inclined ring with a high surface brightness. Past observations have raised several …

Polarimetry with the Gemini planet imager: methods, performance at first light, and the circumstellar ring around HR 4796A

MD Perrin, G Duchene, M Millar-Blanchaer… - The Astrophysical …, 2015 - iopscience.iop.org
We present the first results from the polarimetry mode of the Gemini Planet Imager (GPI),
which uses a new integral field polarimetry architecture to provide high contrast linear …

Keck/NIRC2 L'-band imaging of Jovian-Mass accreting protoplanets around PDS 70

JJ Wang, S Ginzburg, B Ren, N Wallack… - The Astronomical …, 2020 - iopscience.iop.org
We present L'-band imaging of the PDS 70 planetary system with Keck/NIRC2 using the new
infrared pyramid wave front sensor. We detected both PDS 70 b and c in our images, as well …

Collisional processes in extrasolar planetesimal discs–dust clumps in Fomalhaut's debris disc

MC Wyatt, WRF Dent - Monthly Notices of the Royal …, 2002 - academic.oup.com
This paper presents a model for the outcome of collisions between planetesimals in a debris
disc, and assesses the impact of collisional processes on the structure and size distribution …