Early Planet Formation in Embedded Disks (eDisk). I. Overview of the Program and First Results
N Ohashi, JJ Tobin, JK Jørgensen… - The Astrophysical …, 2023 - iopscience.iop.org
We present an overview of the Large Program," Early Planet Formation in Embedded Disks
(eDisk)," conducted with the Atacama Large Millimeter/submillimeter Array (ALMA). The …
(eDisk)," conducted with the Atacama Large Millimeter/submillimeter Array (ALMA). The …
A highly settled disk around oph163131
M Villenave, KR Stapelfeldt, G Duchêne… - The Astrophysical …, 2022 - iopscience.iop.org
High dust density in the midplane of protoplanetary disks is favorable for efficient grain
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
The APOGEE-2 survey of the orion star-forming complex. II. Six-dimensional structure
We present an analysis of spectroscopic and astrometric data from APOGEE-2 and Gaia
DR2 to identify structures toward the Orion Complex. By applying a hierarchical clustering …
DR2 to identify structures toward the Orion Complex. By applying a hierarchical clustering …
A large catalog of accurate distances to local molecular clouds: the Gaia DR2 edition
C Zucker, JS Speagle, EF Schlafly… - The Astrophysical …, 2019 - iopscience.iop.org
We present a uniform catalog of accurate distances to local molecular clouds informed by
the Gaia DR2 data release. Our methodology builds on that of Schlafly et al. First, we infer …
the Gaia DR2 data release. Our methodology builds on that of Schlafly et al. First, we infer …
A compendium of distances to molecular clouds in the Star Formation Handbook
Accurate distances to local molecular clouds are critical for understanding the star and
planet formation process, yet distance measurements are often obtained inhomogeneously …
planet formation process, yet distance measurements are often obtained inhomogeneously …
Early Planet Formation in Embedded Disks (eDisk). VII. Keplerian Disk, Disk Substructure, and Accretion Streamers in the Class 0 Protostar IRAS 16544–1604 in CB …
M Kido, S Takakuwa, K Saigo, N Ohashi… - The Astrophysical …, 2023 - iopscience.iop.org
We present observations of the Class 0 protostar IRAS 16544–1604 in CB 68 from the" Early
Planet Formation in Embedded Disks (eDisk)" ALMA Large program. The ALMA …
Planet Formation in Embedded Disks (eDisk)" ALMA Large program. The ALMA …
The Ophiuchus DIsc Survey Employing ALMA (ODISEA)–I: project description and continuum images at 28 au resolution
LA Cieza, D Ruíz-Rodríguez, A Hales… - Monthly Notices of …, 2019 - academic.oup.com
Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
The Gould's Belt Distances Survey (GOBELINS). II. Distances and structure toward the Orion molecular clouds
We present the results of the Gould's Belt Distances Survey of young star-forming regions
toward the Orion Molecular Cloud Complex. We detected 36 young stellar objects (YSOs) …
toward the Orion Molecular Cloud Complex. We detected 36 young stellar objects (YSOs) …
Recent progress in theory and observational study of dust grain alignment and rotational disruption in star-forming regions
Modern understanding of dust astrophysics reveals that radiative torques (RATs) arising
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
A millimeter Continuum Size–Luminosity Relationship for Protoplanetary Disks
We present a survey at subarcsecond resolution of the 340 GHz dust continuum emission
from 50 nearby protoplanetary disks, based on new and archival observations with the …
from 50 nearby protoplanetary disks, based on new and archival observations with the …