Galaxy Formation and Evolution.  R. B. Larson, 1992, in “Star Formation in Stellar Systems”, lectures presented at a winter school in Tenerife, Spain, December 1991, eds. G. Tenorio-Tagle, M. Prieto, & F. Sanchez  (Cambridge University Press, Cambridge),  p. 125.  (PDF)

Star Formation in Groups.  R. B. Larson, 1995, Monthly Notices Roy. Astron. Soc., 272, 213.  (PDF)

Early Star Formation and the Evolution of the Stellar Initial Mass Function in Galaxies.  R. B. Larson, 1998, Monthly Notices Roy. Astron. Soc., 301, 569.  (PDF)

The Stellar Initial Mass Function: Constraints from Young Clusters, and Theoretical Perspectives.  M. R. Meyer, F. C. Adams, L. A. Hillenbrand, J. M. Carpenter, & R. B. Larson, 2000, in “Protostars and Planets IV”, conference in Santa Barbara, California, July 1998, eds. V. Mannings, A. P. Boss, & S. S. Russell (University of Arizona Press, Tucson),  p. 121.  (PDF)

The Stellar Initial Mass Function.   R. B. Larson, 1999, in “Star Formation 1999”, meeting in Nagoya, Japan, June 1999, ed. T. Nakamoto (Nobeyama Radio Observatory, Nobeyama),  p. 336.  (PDF)

The Stellar Initial Mass Function and Beyond.   R. B. Larson, 2003, in “Galactic Star Formation Across the Stellar Mass Spectrum”, IAOC Workshop in La Serena, Chile, March 2002, eds. J. M. De Buizer & N. S. van der Bliek (ASP Conference Series Vol. 287, ASP, San Francisco),  p. 65.  (PDF)

Understanding the IMF.  R. B. Larson, 2005, in “The Initial Mass Function 50 Years Later”, meeting at Abbazia di Spineto, Siena, Italy, May 2004, eds. E. Corbelli, F. Palla, & H. Zinnecker (Springer, Dordrecht),  p. 329.  (PDF)

The Stellar Mass Spectrum from Non-Isothermal Gravoturbulent Fragmentation.  R. Klessen, K. Jappsen, R. Larson, Y. Li, M.-M. Mac Low, 2005, in “The Initial Mass Function 50 Years Later”, meeting at Abbazia di Spineto, Siena, Italy, May 2004, eds. E. Corbelli, F. Palla, & H. Zinnecker (Springer, Dordrecht),  p. 363.  (PDF)

Thermal Physics, Cloud Geometry, and the Stellar Initial Mass Function.  R. B. Larson, 2005, Monthly Notices Roy. Astron. Soc., 359, 211.  (PDF)

The Stellar Mass Spectrum from Non-Isothermal Gravoturbulent Fragmentation.  A.-K. Jappsen, R. S. Klessen, R. B. Larson, Y. Li, & M.-M. Mac Low, 2005, Astronomy and Astrophysics, 435, 611.  (PDF)

Understanding the Stellar Initial Mass Function.   R. B. Larson, 2006, in “XI IAU Regional Latin American Meeting of Astronomy”, Pucon, Chile, December 2005, eds. L. Infante, M. Rubio, & S. Torres-Peimbert (Revista Mexicana de Astronomia y Astrofisica, Serie de Conferencias, Vol. 26),  p. 55.  (PDF)

The Origin of the Initial Mass Function.  I. A. Bonnell, R. B. Larson, & H. Zinnecker, 2007, in “Protostars and Planets V”, conference at Waikoloa, Hawaii, October 2005, eds. B. Reipurth, D. Jewitt, & K. Keil (University of Arizona Press, Tucson),  p. 149.  (PDF)

Hayashi and the Thermal Physics of Star-Forming Clouds.  R. B. Larson, 2012, in “FIRST STARS IV – From Hayashi to the Future”, meeting in Kyoto, Japan, May 2012, in honor of Chushiro Hayashi, eds. M. Umemura & K. Omukai (AIP Conference Proceedings 1480, Melville, NY),  p. 38.   (PDF)