An analysis of the Herbig star population and their protoplanetary disks within 1 kpc

arXiv:2608.23729 · astro-ph.EP, astro-ph.GA, astro-ph.SR · Submitted 2026-08-24 · Read on arXiv

astro-ph.EP, astro-ph.GA, astro-ph.SR

Submitted: 2026-08-24

Updated: 2026-08-24

Terminology

• Calibration — 11× in this paper · explained in 7 episodes
• Aperture — 5× in this paper · explained in 1 episode
• Metallicity — 3× in this paper · explained in 3 episodes
• Common Astronomy Software Applications — 2× in this paper
• Accretion Flows — 1× in this paper · explained in 1 episode
• Atacama Compact Array — 1× in this paper
• Clustering — 1× in this paper · explained in 2 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Streaming Instability — 1× in this paper · explained in 2 episodes

Sources

• The Ophiuchus DIsc Survey Employing ALMA (ODISEA). Substructures as a function of SED Class and disc mass in 100 systems
• Infall Explains the Disk Kinematics of AB Aur Without Gravitational Instability
• Dust masses of Upper Scorpius disks and their statistics
• X-Shooter survey of disk accretion in Upper Scorpius II. A lack of correlation between accretion rates and disk properties
• The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
• Planet-forming disks and their environment across regions and time from the full NIR census
• Azimuthal molecular variations in the AB Aur planet-forming disk
• Reproducing the stellar-mass dependence of the giant planet occurrence rate with pebble accretion models
• Analysing the SEDs of protoplanetary disks with machine learning
• Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets
• Survival of Protoplanetary Disks in Upper Scorpius from Population Synthesis Models with External Photoevaporation
• Precise determination of circumstellar disk lifetimes: Disk evolution in a single star-forming region
• A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins
• The Circumbinary Disk of HD 34700A: I. CO gas kinematics indicate spirals, infall, and vortex motions
• Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses

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