Massive star formation in 100,000 years from turbulent and pressurized molecular clouds

Author:

McKee Christopher F.,Tan Jonathan C.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference30 articles.

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2. McLaughlin, D. E. & Pudritz, R. E. Gravitational collapse and star formation in logotropic and nonisothermal spheres. Astrophys. J. 476, 750–765 (1997).

3. Stahler, S. W., Palla, F. & Ho, P. T. P. in Protostars & Planets IV (eds Mannings, V., Boss, A. P. & Russell, S. S.) 327–351 (Univ. Arizona Press, Tucson, 2000).

4. Behrend, R. & Maeder, A. Formation of massive stars by growing accretion rate. Astron. Astrophys. 373, 190–198 (2001).

5. Osorio, M., Lizano, S. & D'Alessio, P. Hot molecular cores and the formation of massive stars. Astrophys. J. 525, 808–820 (1999).

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