Papers

Interesting papers can be put here. Please:

• Indicate the title and some author information
• Put a link to the abstract page, not to the PDF (better for many reasons)
• Within a subject, sort by descending chronological order of addition (i.e., newest on top)
• Put comments and discussions on the page Discussion.

Enjoy reading!

Stars

• Balmer et al. 2023, "VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”"

• Young 2023, "Insights into the first and second hydrostatic core stages from numerical simulations"

• López-Vázquez et al., "Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow"

Discs

• Fenton & Stamatellos 2024, "The 3D structure of disc-instability protoplanets"

• Takakuwa et al. 2024, "Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a"

• Ren et al. 2024, "A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion"

• Lim et al 2023, "Streaming Instability and Turbulence: Conditions for Planetesimal Formation"

• Jiang et al. 2023, "Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks"

• Ashraf et al. 2023, "An outburst and FU Ori-type disk of a former low luminosity protostar"

• Guadarrama et al. 2023, "The influence of accretion bursts on methanol and water in massive young stellar objects"

• Fuksman et al. 2023, "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating"

• Fuksman et al. 2023, "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions"

• Higginbottom et al., "State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows"

• Nixon et al., "On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos"

• Stapper et al., "Constraining the gas mass of Herbig disks using CO isotopologues"

• Paneque-Carreño et al., "High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission"

• Chen et al., "Planet Gap-opening Feedback on Disk Thermal Structure and Composition"

• Cattolico & Perets, "Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems"

Planets

• Krapp et al. 2024, "A thermodynamic criterion for the formation of Circumplanetary Disks"

• Andama et al. 2024, "What stars can form planets: planetesimal formation at low"

• Law et al. 2024, "Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk"

• Lorek & Johansen 2024, "Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds"

• Burn et al. 2024, "A radius valley between migrated steam worlds and evaporated rocky cores"

• Jones et al. 2024, "A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS"

• Xu & Wang 2024, "Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures"

• Portegies Zwart & Hochart, "The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters"

Small things

• Birnstiel 2023, "Dust growth and evolution in protoplanetary disks"

• Dominik and Dullemond 2023, "The bouncing barrier revisited: Impact on key planet formation processes and observational signatures"

• Houge et al., "Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles"

Other (including ornithology)

• Van Wassenbergh & Mielke (2024), "Why woodpeckers don’t get concussions", Physics Today (short read)
• Dib & Menou, "Physics simulation capabilities of LLMs"
• Keto (2020), Stability and solution of the time-dependent Bondi–Parker flow