Papers to read

The page is to mimic Dong’s group meeting paper page. (PS: right-click on the links to read in new tabs.)

Week of Jan 13, 2025

• Fri Jan 17, 2025
  • REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths
  • Spin-Orbit Alignment in Merging Binary Black Holes Following Collisions with Massive Stars
  • A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054
  • Resolving the χeff-q correlation among Coalescing Binary Black Holes and Evidence for AGN-driven Hierarchical Mergers
• Thu Jan 16, 2025
  • Complex Structure around a Circumstellar Disk Caused by Interchange Instability
  • Discovery of a years-delayed radio flare from an unusually slow-evolved tidal disruption event
  • Empirical Constraints on Tidal Dissipation in Exoplanet Host Stars
  • Prompt gravitational-wave mergers aided by gas in Active Galactic Nuclei: The hydrodynamics of binary-single black hole scatterings
• Wed Jan 15, 2025
  • Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
  • The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks: Scale-dependence of dust diffusion
  • High-Contrast Imaging: Hide and Seek with Exoplanets
  • Global 3-D Simulations of Magnetospheric Accretion: II. Hot Spots, Equilibrium Torque, Episodic Wind, and Midplane Outflow
  • Architecture Classification for Extrasolar Planetary Systems
  • Vertical CO surfaces as a probe for protoplanetary disk mass and carbon depletion
• Tue Jan 14, 2025
  • From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability
  • Stellar Population and Metal Production in AGN Disks
  • Is planetary inward migration responsible for GJ 504’s fast rotation and bright X-ray luminosity? New constraints from eROSITA
  • Dusty disk as a safe haven for terrestrial planets: Effect of back-reaction of solid material on gas
  • Three-dimensional transport of solids in a protoplanetary disk containing a growing giant planet
• Mon Jan 13, 2025
  • Planet formation and long-term stability in a very eccentric stellar binary
  • The 2D pressure structure of the HD 163296 protoplanetary disk as probed by multi-molecular kinematics
  • Stellar obliquities of eight close-in gas giant exoplanets
  • Extreme exomoons in WASP-49 Ab: dynamics and detectability
  • Smuggling unnoticed: Towards a 2D view of water and dust delivery to the inner regions of protoplanetary discs
  • Dust processing in the terrestrial planet-forming region of the PDS 70 disk
  • Modeling the Impact of Moderate External UV Irradiation on Disk Chemistry

Week of Jan 06, 2025

• Fri Jan 10, 2025
  • Orbits of Six Triple Systems
  • *On vertical variations of gas flow in protoplanetary disks and their impact on the transport of solids
• Thu Jan 09, 2025
  • Detecting Exomoons in Free-Floating-Planet Events from Space-based Microlensing Surveys
  • Accretion disc winds imprint distinct signatures in the optical variability spectrum of black hole transients
  • LAMOST Reveals Long-lived Protoplanetary Disks
  • Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES
  • The evolution of the flux-size relationship in protoplanetary discs by viscous evolution and radial pebble drift
  • MINDS. The influence of outer dust disc structure on the volatile delivery to the inner disc
• Wed Jan 08, 2025
  • Science Opportunities of Wet Extreme Mass-Ratio Inspirals
  • Stellar Tidal Disruptions by Newborn Neutron Stars or Black Holes: A Mechanism for Hydrogen-poor (Super)luminous Supernovae and Fast Blue Optical Transients
  • Formation of super-Earths and mini-Neptunes from rings of planetesimals
  • ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) VII: the layered molecular outflow from HL Tau and its relationship with the ringed disk
• Tue Jan 07, 2025
  • Statistical trends in JWST transiting exoplanet atmospheres
  • Dynamics of the Beta Pictoris planetary system and possibility of an additional planet
• Mon Jan 06, 2025
  • Sequencing Silicates in the IRS Debris Disk Catalog I: Methodology for Unsupervised Clustering
  • Millihertz Oscillations Near the Innermost Orbit of a Supermassive Black Hole
  • Exoplanet Detection via Differentiable Rendering

Week of Dec 30, 2024

• Fri Jan 03, 2025
  • Exchange of meteorites between the terrestrial planets and the Moon
  • A Planet as the Possible Cause of the HD 181327 Debris Disk Asymmetry
• Tue Dec 31, 2024
• Mon Dec 30, 2024
  • Secular Perturbations from Exterior Giants Strongly Influence Gap Complexity in Peas-in-a-Pod Exoplanetary Systems

Week of Dec 23, 2024

• Tue Dec 24, 2024
  • Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation
• Mon Dec 23, 2024
  • Observational Signatures of Disk Winds in Protoplanetary Disks: Differentiating Magnetized and Photoevaporative Outflows With Fully Coupled Thermochemistry

Week of Dec 16, 2024

• Fri Dec 20, 2024
  • Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Dynamical Evidence of a Spiral-Arm-Driving and Gap-Opening Protoplanet from SAO 206462 Spiral Motion
  • Shedding light on the origin of the broken misaligned circumtriple disk around GW Ori
• Thu Dec 19, 2024
  • Evolution of orbits of trans-Neptunian bodies at the 2:3 resonance with Neptune
  • The Hottest Neptunes Orbit Metal-Rich Stars
  • Streaming Torque with Turbulent Diffusion
  • On the maximum disk heating attributable to fuzzy dark matter
• Wed Dec 18, 2024
  • *Creating Pileups of Eccentric Planet Pairs Wide of MMRs Through Divergent Migration
  • MINDS. JWST-MIRI reveals a peculiar CO2-rich chemistry in the drift-dominated disk CX Tau
  • The Galactic Disk North-south Asymmetry in Metallicity May Be A New Tracer for the Disk Warp
  • Variations in orbital elements of planets
  • Anisotropic tidal dissipation in misaligned planetary systems
• Tue Dec 17, 2024
  • *Circumbinary accretion as a diagnostic for binary–disc misalignment
  • Dust Scattering Albedo at Millimeter-Wavelengths in the TW Hya Disk
  • Planet formation theory: an overview
  • Vortex-Induced Rings and Gaps within Protoplanetary Disks
  • Combined analysis of the 12.8 and 15 μm JWST/MIRI eclipse observations of TRAPPIST-1 b
  • Evidence for the spin-kick alignment of pulsars from the statistics of their magnetic inclinations
  • Black Hole Merger Rates in AGN: contribution from gas-captu
• Mon Dec 16, 2024
  • Vertical Shear Instability in Thermally-Stratified Protoplanetary Disks: I. A Linear Stability Analysis
  • Vertical Shear Instability in Thermally-Stratified Protoplanetary Disks: II. Hydrodynamic Simulations and Observability

Week of Dec 9, 2024

• Fri Dec 13, 2024
  • *The Spin-Orbit Alignment of 8 Warm Gas Giant Systems
  • Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: I. Free-floating MLPs
  • Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581
  • Journey of complex organic molecules: Formation and transport in protoplanetary disks
  • Asymmetric Temperature Variations In Protoplanetary disks: I. Linear Theory and Corotating Spirals
• Thu Dec 12, 2024
  • Probing the gas that builds planets: Results from the JWST MINDS program
  • An Obliquity Measurement of the Hot Neptune TOI-1694b
• Wed Dec 11, 2024
  • On the kinematic and thermodynamic state of clouds in complex wind-multi-cloud environments using a Friends-of-Friends analysis
  • *Linear bending wave propagation in laminar and turbulent discs
  • Simultaneous emission from dust and gas in the planetary debris orbiting a white dwarf
• Tue Dec 10, 2024
  • A potential exomoon from the predicted planet obliquity of β Pictoris b
  • Dissecting the disk and the jet of a massive (proto)star. An ALMA view of IRAS20126+4104
  • On the formation of super-Jupiters: Core Accretion or Gravitational Instability?
• Mon Dec 9, 2024
  • Machine learning approach for mapping the stable orbits around planets
  • A substellar flyby that shaped the orbits of the giant planets
  • Chondrites as thermal and mechanical archives of accretion processes in the Solar protoplanetary disk
  • The effect of radiation pressure on the dispersal of photoevaporating discs
  • The Origin and Evolution of Saturn: A Post-Cassini Perspective

Week of Dec 2, 2024

• Fri Dec 6, 2024
  • Predictions of Dust Continuum Emission from a Potential Circumplanetary Disk: A Case Study of the Planet Candidate AB Aurigae b
  • Investigating Kozai-Lidov Oscillations and Disc Tearing in Be Star Discs
  • Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral
  • From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest Mp/M∗ Systems Exhibit Low Obliquities, Even around Hot Stars
• Thu Dec 5, 2024
  • Discovery and Characterization of an Eccentric, Warm Saturn Transiting the Solar Analog TOI-4994
  • Exomoons of Circumbinary Planets
  • Angular Momentum Drain: Despinning Embedded Planetesimals
• Wed Dec 4, 2024
  • Late-time Evolution and Instabilities of Tidal Disruption Disks
  • Gravitational wave mergers of accreting binary black holes in AGN discs
  • Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
  • Forming Earth-like and Low-Mass Rocky Exoplanets Through Pebble and Planetesimal Accretion
• Tue Dec 3, 2024
  • Disk-Locking Regulates Stellar Rotation in Young Clusters: Insights from NGC 2264
  • Origins of rings in the solar system
  • Formation Rate of Quasi-periodic Eruptions in Galactic Nuclei Containing Single and Dual Supermassive Black Holes
  • Hydrodynamical simulations of proto-Moon degassing
  • An impact-free mechanism to deliver water to terrestrial planets and exoplanets
  • Concealing Circumbinary Planets with Tidal Shrinkage
  • The Yarkovsky effect on the long-term evolution of binary asteroids
• Mon Dec 2, 2024
  • A giant planet transiting a 3-Myr protostar with a misaligned disk
  • Orbital Migration through Atmospheric Mass Loss
  • Hydrodynamical simulations with strong indirect terms in Fargo-like codes: Numerical aspects of non-inertial frame and artificial viscosity
  • Methods to Characterise Exoplanet Host Stars from Spectroscopy
  • Long-term stability and dynamical spacing of compact planetary systems

Week of Nov 25, 2024

• Fri Nov 29, 2024: Thanksgiving (no arXiv update)
• Thu Nov 28, 2024
  • A Measurement of the Water Abundance in the Atmosphere of the Hot Jupiter WASP-43b with High-resolution Cross-correlation Spectroscopy
• Wed Nov 27, 2024
  • Mixed origins: strong natal kicks for some black holes and none for others
  • A possible misaligned orbit for the young planet AU Mic c
  • Revisiting the conundrum of the sub-Jovian and Neptune desert. A new approach that incorporates stellar properties
  • Comment on “Did the terrestrial planets of the Solar System form by pebble accretion?”
  • Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disk
  • Kinetic Field Theory Applied to Planetesimal Formation I: Freely Streaming Dust Particles
  • Validating the Orbital Periods of the Coolest TESS Exoplanet Candidates
• Tue Nov 26, 2024
  • Simulations of Eccentricity Growth in Compact Binary Accretion Disks with MHD Turbulence
  • Once a giant, (almost) always a giant: Partial Tidal Disruption Events of Giant Stars
  • Circumbinary disks in post-common envelope binary systems with compact objects
  • The fate of EMRI-IMRI pairs in AGN accretion disks: long-term simulations
• Mon Nov 25, 2024
  • Pebble Accretion
  • The Moon-forming Impact as a Constraint for the Inner Solar System’s Formation
  • Stochastic acceleration in arbitrary astrophysical environments
  • PDS 70b Shows Stellar-like Carbon-to-Oxygen Ratio

Week of Nov 18, 2024

• Fri Nov 22, 2024
  • Planets Around Solar Twins/Analogs (PASTA) I.: High precision stellar chemical abundance for 17 planet-hosting stars and the condensation temperature trend
  • Collisional damping in debris discs: Only significant if collision velocities are low
  • Observing planetary gaps in the gas of debris disks
• Thu Nov 21, 2024
  • Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks
  • Streams and Bubbles: Tidal Shaping of Planetary Outflows
  • Understanding the UV/Optical Variability of AGNs through Quasi-Periodic Large-scale Magnetic Dynamos
  • Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and VLA Observations
  • Impact of Jupiter’s heating and self-shadowing on the Jovian circumplanetary disk structure
  • Small and Close-In Planets are Uncommon around A-type Stars
  • Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 069
  • Accreting Binary Eccentricities follow Predicted Equilibrium Values
• Wed Nov 20, 2024
  • Light Echoes of Protoplanetary Disks
  • Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows
  • Observational Signatures of Dust Traffic Jams in Polar-Aligning Circumbinary Disks
  • Planet-planet scattering in systems of multiple planets of unequal mass