The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?

The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?DOI: info:10.3847/2041-8213/abe7ddv. 910L6
Takemura, Hideaki, Nakamura, Fumitaka, Kong, Shuo, Arce, Héctor G., Carpenter, John M., Ossenkopf-Okada, Volker, Klessen, Ralf, Sanhueza, Patricio, Shimajiri, Yoshito, Tsukagoshi, Takashi, Kawabe, Ryohei, Ishii, Shun, Dobashi, Kazuhito, Shimoikura, Tomomi, Goldsmith, Paul F., Sánchez-Monge, Álvaro, Kauffmann, Jens, Pillai, Thushara G. S., Padoan, Paolo, Ginsberg, Adam, Smith, Rowan J., Bally, John, Mairs, Steve, Pineda, Jaime E., Lis, Dariusz C. et al. 2021. "The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?" The Astrophysical Journal, 910 L6. https://doi.org/10.3847/2041-8213/abe7dd.
ID: 159427
Type: article
Keywords: SAO