About: Aaron C. Boley

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

researcher (ORCID 0000-0002-0574-4418)

Attributes	Values
rdf:type	Item
description	باحث (معرف أورسيد 0000-0002-0574-4418) (ar) researcher (ORCID 0000-0002-0574-4418) (en)
rdfs:label	Aaron C. Boley (en)
skos:prefLabel	Aaron C. Boley (en)
name	Aaron C. Boley (en)
given name	wds:Q111975854-7b08268a-4054-3bc9-14e3-8b20315d7ea9 wds:Q111975854-c73676c3-460e-b88c-1fce-59cd63b8c575
given name	Aaron Christopher
instance of	wds:Q111975854-b434bba6-41ab-be70-64c2-99402de00df4
instance of	Homo sapiens
doctoral advisor	wds:Q111975854-b8f00756-4e63-7740-89a5-096d28cad7d4
Academic Tree ID	wds:Q111975854-B9C503D2-2A9F-4A47-AE76-1682391A5BE4
Mathematics Genealogy Project ID	wds:Q111975854-3d6934bd-4e3b-bf6f-3852-9d37d287ab88
doctoral advisor	Richard H. Durisen
Academic Tree ID	199990
Mathematics Genealogy Project ID	295341
AstroGen ID	wds:Q111975854-D3D74D73-567D-4996-AEAE-05488A64F804
AstroGen ID	2126
skos:altLabel	A Boley (en) A C Boley (en) A. Boley (en) A. C. Boley (en) A.C. Boley (en) Aaron Boley (en) Aaron C Boley (en) Aaron Christopher Boley (fr)
occupation	wds:Q111975854-1dd8bf6c-432f-60f7-e81a-93740dd289e5
employer	wds:Q111975854-7EACB1F6-E779-4315-9E7E-FAEC2D760F0F
sex or gender	wds:Q111975854-375372a4-421b-5a6b-e3b1-83b0813acd87
VIAF ID	wds:Q111975854-08189824-b3f6-40a2-a12d-0bccb2368c70
Library of Congress authority ID	wds:Q111975854-c82ecb39-4607-0e90-81fc-7e5d10d3b3e9
member of	wds:Q111975854-3D8AA1D5-96B7-4B5F-BF43-A54A32F572D3
educated at	wds:Q111975854-b97c63d3-4e3c-4247-2855-dc45cddcd4cb
family name	wds:Q111975854-2574574F-383D-4EC9-8AE0-FA5EC4A4A152
VIAF ID	http://viaf.org/viaf/28166234275396042474
Library of Congress authority ID	http://id.loc.gov/authorities/names/n2022046085
occupation	astronomer
employer	University of British Columbia Vancouver campus
sex or gender	male
VIAF ID	28166234275396042474
Library of Congress authority ID	n2022046085
member of	International Astronomical Union
educated at	Indiana University Bloomington
family name	Boley
ORCID iD	wds:Q111975854-980d8807-4423-90a1-7cec-322eefa1da62
ORCID iD	https://orcid.org/0000-0002-0574-4418
ORCID iD	0000-0002-0574-4418
IAU member ID	wds:Q111975854-6F3D5DB5-CF1A-4EB2-8028-4274E25D526D
IAU member ID	16095
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q111975854
is author of	Gravitational instabilities in a protosolar-like disc – I. Dynamics and chemistry Three-dimensional radiative hydrodynamics for disk stability simulations: a proposed testing standard and new results Chemistry in a gravitationally unstable protoplanetary disc Convergence studies of mass transport in disks with gravitational instabilities. I. The constant cooling time case The in situ formation of giant planets at short orbital periods Constraining the planetary system of Fomalhaut using high-resolution ALMA observations Transit Duration Variations in Multiplanet Systems Sustainable skies and the Earth–space environment Simulations of small solid accretion on to planetesimals in the presence of gas The thermal regulation of gravitational instabilities in protoplanetary disks. III. Simulations with radiative cooling and realistic opacities Hydraulic/shock jumps in protoplanetary disks Resolved CO gas interior to the dust rings of the HD 141569 disk Magnetic fields recorded by chondrules formed in nebular shocks U.S. policy puts the safe development of space at risk Overcoming the meter barrier and the formation of systems with tightly packed inner planets (STIPs) The effects of metallicity and grain size on gravitational instabilities in protoplanetary disks Globular cluster formation within a cosmological context High-temperature processing of solids through solar nebular bow shocks: 3D radiation hydrodynamics simulations with particles Gravitational instabilities, chondrule formation, and the FU Orionis phenomenon 1.3-mm ALMA observations of the Fomalhaut debris system The dynamics of tightly-packed planetary systems in the presence of an outer planet: case studies using Kepler-11 and Kepler-90 Planetary embryo bow shocks as a mechanism for chondrule formation Core-assisted gas capture instability: a new mode of giant planet formation by gravitationally unstable discs MESAS: Measuring the Emission of Stellar Atmospheres at Submillimeter/millimeter Wavelengths Apophis 2029: Decadal Opportunity for the Science of Planetary Defense The evolution of circumplanetary disks around planets in wide orbits: implications for formation theory, observations, and moon systems The MESAS Project: Long-wavelength Follow-up Observations of Sirius A Extended millimeter emission in the HD 141569 circumstellar disk detected with ALMA On shocks driven by high-mass planets in radiatively inefficient disks. II. Three-dimensional global disk simulations The internal energy for molecular hydrogen in gravitationally unstable protoplanetary disks The thermal regulation of gravitational instabilities in protoplanetary disks. IV. Simulations with envelope irradiation Convergence studies of mass transport in disks with gravitational instabilities. II. The radiative cooling case The Case for Space Environmentalism The heavy-element composition of disk instability planets can range from sub- to super-nebular On the possibility of enrichment and differentiation in gas giants during birth by disk instability The chemistry of protoplanetary fragments formed via gravitational instabilities Chondrule formation in bow shocks around eccentric planetary embryos Gravitational instabilities in a protosolar-like disc III: molecular line detection and sensitivities On shocks driven by high-mass planets in radiatively inefficient disks. I. Two-dimensional global disk simulations On the origin of banded structure in dusty protoplanetary disks: HL Tau and TW Hya Visibility Predictions for Near-future Satellite Megaconstellations: Latitudes near 50° Will Experience the Worst Light Pollution ALMA and VLA observations of the HD 141569 system The MESAS Project: ALMA Observations of the F-type Stars γ Lep, γ Vir A, and γ Vir B Plaskett 1.8 m Observations of Starlink Satellites Migration of gas giant planets in gravitationally unstable disks Interactions between moderate- and long-period giant planets: scattering experiments for systems in isolation and with stellar flybys Gravitational instabilities in a protosolar-like disc – II. Continuum emission and mass estimates The two modes of gas giant planet formation

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