The core mass function in the Orion Nebula Cluster region: What Determines the Final Stellar Masses?

Hideaki Takemura, Fumitaka Nakamura, Shuo Kong, Héctor G. Arce, John M. Carpenter, Volker Ossenkopf-Okada, Ralf Klessen, Patricio Sanhueza, Yoshito Shimajiri, Takashi Tsukagoshi, Ryohei Kawabe, Shun Ishii, Kazuhito Dobashi, Tomomi Shimoikura, Paul F. Goldsmith, Álvaro Sánchez-Monge, Jens Kauffmann, Thushara Pillai, Paolo Padoan, Adam GinsbergRowan J. Smith, John Bally, Steve Mairs, Jaime E. Pineda, Dariusz C. Lis, Blakesley Burkhart, Peter Schilke, Hope How-Huan Chen, Andrea Isella, Rachel K. Friesen, Alyssa A. Goodman, Doyal A. Harper

Research output: Contribution to journalArticlepeer-review

Fingerprint

Dive into the research topics of 'The core mass function in the Orion Nebula Cluster region: What Determines the Final Stellar Masses?'. Together they form a unique fingerprint.

Physics