Lachlan Lancaster

Physics and Astronomy · Physical Sciences

12h-index772citations43works3.82yr avg
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Research Topics

Stellar, planetary, and galactic studies(16), Astronomy and Astrophysical Research(14), Galaxies: Formation, Evolution, Phenomena(13), Astrophysics and Star Formation Studies(12), Gamma-ray bursts and supernovae(7)

Publications43 total

Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z=7, up to z= 14
ArXiv.org·2026Open Access
Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z=7, up to z= 14
arXiv (Cornell University)·2026Open Access
Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus
The Astrophysical Journal·2026Open Access
Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus
arXiv (Cornell University)·2025Open Access
Density-modulated star formation efficiency: implications for the observed abundance of ultraviolet luminous galaxies at <i>z</i> &amp;gt; 10
Monthly Notices of the Royal Astronomical Society·2025· 10 citedOpen Access
The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. II. 3D RMHD Simulations and Tests of Semianalytic Models
The Astrophysical Journal·2025· 3 citedOpen Access
The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. I. Physical Principles and a Semianalytic Model
The Astrophysical Journal·2025· 2 citedOpen Access
Suppression of Shock X-Ray Emission in Novae from Turbulent Mixing with Cool Gas
The Astrophysical Journal·2025· 1 citedOpen Access
The Co-Evolution of Stellar Wind-blown Bubbles and Photoionized Gas I: Physical Principles and a Semi-Analytic Model
arXiv (Cornell University)·2025Open Access
The Co-Evolution of Stellar Wind-blown Bubbles and Photoionized Gas II: 3D RMHD Simulations and Tests of Semi-Analytic Models
arXiv (Cornell University)·2025Open Access
Suppression of Shock X-ray Emission in Novae from Turbulent Mixing with Cool Gas
arXiv (Cornell University)·2025Open Access
Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z&gt;10
arXiv (Cornell University)·2025Open Access
Detection of Diffuse Hot Gas around the Young, Potential Superstar Cluster H72.97–69.39
The Astrophysical Journal·2024· 2 citedOpen Access
Geometry, Dissipation, Cooling, and the Dynamical Evolution of Wind-blown Bubbles
The Astrophysical Journal·2024· 19 citedOpen Access
The Interplay between the Initial Mass Function and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities
The Astrophysical Journal Letters·2024· 30 citedOpen Access
Geometry, Dissipation, Cooling, and the Dynamical Evolution of Wind-Blown Bubbles
arXiv (Cornell University)·2024Open Access
The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities
arXiv (Cornell University)·2024· 1 citedOpen Access
Detection of Diffuse Hot Gas Around the Young, Potential Superstar Cluster H72.97-69.39
arXiv (Cornell University)·2024Open Access
Structure, Kinematics, and Observability of the Large Magellanic Cloud’s Dynamical Friction Wake in Cold versus Fuzzy Dark Matter
The Astrophysical Journal·2023· 18 citedOpen Access
Structure, Kinematics, and Observability of the Large Magellanic Cloud's Dynamical Friction Wake in Cold vs. Fuzzy Dark Matter
arXiv (Cornell University)·2023Open Access
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Frequent Co-authors

Chang‐Goo Kim(9), Philip Mocz(8), Mark Vogelsberger(7), S. E. Koposov(7), Eve C. Ostriker(7), Jeong‐Gyu Kim(7), Shyam H. Menon(6), Greg L. Bryan(6), Anastasia Fialkov(5), Pierre-Henri Chavanis(5), Vasily Belokurov(5), Jenny E. Greene(5), Mustafa A. Amin(4), Sownak Bose(4), Michael Boylan-Kolchin(4), Lars Hernquist(4), Victor H. Robles(4), Alis J. Deason(4), Laura Sommovigo(4), Trinity L. Webb(4)