Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation
CF Manara, M Ansdell, GP Rosotti, AM Hughes… - arXiv preprint arXiv …, 2022 - arxiv.org
Since Protostars and Planets VI (PPVI), our knowledge of the global properties of
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …
Debris disks: structure, composition, and variability
AM Hughes, G Duchêne… - Annual Review of …, 2018 - annualreviews.org
Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …
wide range of ages. Those around main sequence stars are analogous to the Solar System's …
A kinematical detection of two embedded Jupiter-mass planets in HD 163296
We present the first kinematical detection of embedded protoplanets within a protoplanetary
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
Molecules with ALMA at Planet-forming Scales (MAPS). II. CLEAN strategies for synthesizing images of molecular line emission in protoplanetary disks
The Molecules with ALMA at Planet-forming Scales Large Program (MAPS LP) surveyed the
chemical structures of five protoplanetary disks across more than 40 different spectral lines …
chemical structures of five protoplanetary disks across more than 40 different spectral lines …
CO depletion in protoplanetary disks: a unified picture combining physical sequestration and chemical processing
The gas-phase CO abundance (relative to hydrogen) in protoplanetary disks decreases by
up to two orders of magnitude from its interstellar medium value of∼ 10− 4, even after …
up to two orders of magnitude from its interstellar medium value of∼ 10− 4, even after …
Gas disk sizes from CO line observations: a test of angular momentum evolution
The size of a disk encodes important information about its evolution. Combining new
Submillimeter Array observations with archival Atacama Large Millimeter/submillimeter …
Submillimeter Array observations with archival Atacama Large Millimeter/submillimeter …
Magma ocean, water, and the early atmosphere of Venus
The current state and surface conditions of the Earth and its twin planet Venus are drastically
different. Whether these differences are directly inherited from the earliest stages of …
different. Whether these differences are directly inherited from the earliest stages of …
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 …
characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager …
Temperature, mass, and turbulence: A spatially resolved multiband non-lte analysis of cs in tw hya
R Teague, T Henning, S Guilloteau… - The Astrophysical …, 2018 - iopscience.iop.org
Observations of multiple rotational transitions from a single molecule allow for unparalleled
constraints on the physical conditions of the emitting region. We present an analysis of CS in …
constraints on the physical conditions of the emitting region. We present an analysis of CS in …
Solution to the debris disc mass problem: planetesimals are born small?
AV Krivov, MC Wyatt - Monthly Notices of the Royal Astronomical …, 2021 - academic.oup.com
Debris belts on the periphery of planetary systems, encompassing the region occupied by
planetary orbits, are massive analogues of the Solar system's Kuiper belt. They are detected …
planetary orbits, are massive analogues of the Solar system's Kuiper belt. They are detected …