THE 2014 ALMA LONG BASELINE CAMPAIGN: FIRST RESULTS FROM HIGH ANGULAR RESOLUTION OBSERVATIONS TOWARD THE HL TAU REGION

By Alma Partnership, C. Brogan, L. Pérez, T. Hunter, W. Dent, A. Hales, R. Hills, S. Corder, E. Fomalont, C. Vlahakis and 75 more. 2015

646 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/dd949caae2d0ee1b320b0cda2dd8757ca7466f2c

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Citations in the corpus

The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks (2018, background): “Since the multi-ringed disk observation of HL Tau (ALMA Partnership et al. 2015) a number of such multi-ringed disks have been detected (Andrews et al. 2016; Isella et al. 2016; Cieza et al. 2017; Fedele et al. 2017, 2018; Dipierro et al. 2018; van Terwisga et al. 2018; Clarke et al. 2018; Long et…”
The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation (2018, background): “…the protoplanetary disks down to astronomical unit scales, and a variety of disk features (such as gaps, rings, spirals, and largescale asymmetries) have been revealed (e.g., Casassus et al. 2013; van der Marel et al. 2013; ALMA Partnership et al. 2015; Andrews et al. 2016; Garufi et al. 2017).”
Multiple Disk Gaps and Rings Generated by a Single Super-Earth (2017, methodology): “To date, two systems, HL Tau (ALMA Partnership et al. 2015) and TW Hya (Andrews et al. 2016; Tsukagoshi et al. 2016), have been observed by ALMA with sub-0′′.05 resolution.”
Planetesimal formation near the snowline: in or out? (2017, background): “Such annuli of solid enhancement can be observable with facilities as ALMA.”
Close-in planetesimal formation by pile-up of drifting pebbles (2016, background): “All the panels share a common colour map for convenience. suggest that axisymmetric pile-ups of pebbles occur at various distances from the central star (ALMA Partnership et al. 2015; Andrews et al. 2016).”
Dust Evolution and the Formation of Planetesimals (2016, background): “Recently ALMA observations revealed an intriguing image of a circumstellar disk in HL Tau (ALMA Partnership et al. 2015) which is a Class I young stellar object, earlier than the typical Class II T Tauri stars.”
Why do protoplanetary disks appear not massive enough to form the known exoplanet population? (2018, background): “Also, the rings observed in the disk around the still embedded <1 Myr old HL Tau protostar (ALMA Partnership et al. 2015) may be carved by the presence of planets (e.g., Dipierro et al. 2015) suggesting, again, early planet formation.”
ALMA unveils rings and gaps in the protoplanetary system HD 169142: signatures of two giant protoplanets (2017, background): “…radial (gaps and cavities) and azimuthal (traps and vortices) dust distributions (e.g., Casassus et al. 2012; van der Marel et al. 2013; ALMA Partnership et al. 2015; Walsh et al. 2014; Andrews et al. 2016; Isella et al. 2016) and cold gas cavities that are smaller than the dust cavities…”
Shadows and spirals in the protoplanetary disk HD 100453 (2016, methodology): “Such a difference in the gas kinematics will likely be tested by forthcoming ALMA observations of HD 100453.”
A Kinematical Detection of Two Embedded Jupiter-mass Planets in HD 163296 (2018, background): “…the Atacama Large Millimetre Array (ALMA) has revealed a variety of substructure in continuum emission from protoplanetary disks suggestive of planet-disk interactions sculpting the dust density distribution (ALMA Partnership et al. 2015; Andrews et al. 2016; Isella et al. 2016; Zhang et al. 2016).”
On the diversity and statistical properties of protostellar discs (2018, background): “Although young inner holes have been found recently in discs that are thought to be young (e.g. HL Tau: ALMA Partnership et al. 2015; WL 17: Sheehan & Eisner 2017), in the simulations analysed in this paper the inner holes are certainly numerical, due to the sink particle accretion radius.”
Kinematic Evidence for an Embedded Protoplanet in a Circumstellar Disk (2018, background): “The Atacama Large Millimetre Array (ALMA), and adaptive optics systems have revealed a variety of structures: gaps and rings (ALMA Partnership et al. 2015; Andrews et al. 2016; Isella et al. 2016), spirals (e.g. Benisty et al. 2015; Stolker et al. 2016), that could be signposts of planets, but…”
The Disk Substructures at High Angular Resolution Project (DSHARP). II. Characteristics of Annular Substructures (2018, methodology): “This naming convention is adapted from that used for HL Tau in ALMA Partnership et al. (2015).”