"The Structure and Evolution of Molecular Clouds: from Clumps to Cores to the IMF" | "The Structure and Evolution of Molecular Clouds: from Clumps to Cores to the IMF" |
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"Why the Smallest Stars Stay Small" | "The Fate of the Molecular Gas from Mergers to Ellipticals" |
Birth, Evolution and Death of Stars.
19"On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning | Tracing H 2 Via Infrared Dust Extinction |
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An Introduction to the Theory of Stellar Structure and Evolution |
"On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning.
II — Characteristics of discrete features" | "Why the Smallest Stars Stay Small" |
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Dynamics of Galaxies and Their Molecular Cloud Distributions: Proceedings of the 146th Symposium of the International Astronomical Union | The Astronomy and Astrophysics Review |
Paris, France: Kluwer Academic Publishers.