A real example: what you get
6 new papers close to the project “Observing Planetary Gaps in the Gas of Debris Disks”, found in the announcements of its first days
- How close it is on each facet: question, method, data, results
- What it shares with your project and what stays your own
- What to do: cite it, set your project apart, contact the authors, hurry
- The prior art of the last three years, and the new papers of the teams you name
Partial overlap
The paper investigates resolved CO cavities in transition disks and considers massive planetary companions as a possible explanation. Its isotopologue-dependent cavity sizes provide a relevant observational comparison for interpreting planetary clearing through CO emission.
CO gaps in cold transition disks around low-mass stars
What stays your own
The project instead tests planet-driven gaps and velocity kinks in gas-bearing debris disks using hydrodynamics, radiative transfer, and simulated observations. Its debris-disk detectability criterion and application to HD 138813 remain distinct from this observational study, which does not establish a planetary origin for the cavities.
The email you would have received · 6 new papers are close to your projects
The first results
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CO gaps in cold transition disks around low-mass stars
Partial overlap
The paper investigates resolved CO cavities in transition disks and considers massive planetary companions as a possible explanation. Its isotopologue-dependent cavity sizes provide a relevant observational comparison for interpreting planetary clearing through CO emission.
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CO gaps in cold transition disks around low-mass stars
Partial overlap
This appears to be the published counterpart of the listed Rota et al. preprint, examining CO cavities in three transition disks and discussing a possible planetary explanation. It offers the same relevant comparison between gas depletion and its appearance in …
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Simulation of a Jovian Planet Undergoing Gas Accretion
Partial overlap
Both studies use FARGO3D simulations of giant-planet–disk interactions and examine gas-gap formation while varying planetary orbital radius. This paper studies a two-Jupiter-mass planet in a protoplanetary disk, emphasizing migration and its dependence on initial radius.
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How Eccentric is the Debris Disk of ϵ Eridani? ALMA Reveals a Near-circular Belt
Partial overlap
Both studies investigate how debris-disk structures can constrain otherwise unseen planets. This paper uses the eccentricity of the dust belt around ϵ Eridani, together with imaging constraints, to limit possible planetary architectures.
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Kinematic Signatures of Stellar Flybys in Protoplanetary Discs
Partial overlap
Both studies use hydrodynamical simulations and synthetic ALMA CO observations to investigate observable gas-kinematic signatures of gravitational perturbations in circumstellar disks. The flyby study provides relevant context for interpreting non-Keplerian features without uniquely attributing them to planets.
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Dynamical Impacts of Accretion Streamers on Protoplanetary Disks
Partial overlap
Both studies use hydrodynamic simulations and synthetic ALMA molecular-line observations to investigate observable disk velocity disturbances. The streamer study identifies a nonplanetary source of kinematic signatures, relevant to interpreting proposed planetary kinks.
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