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2021ApJ...910L...6T - Astrophys. J., 910, L6-L6 (2021/March-3)
The core mass function in the Orion Nebula Cluster region: what determines the final stellar masses?
TAKEMURA H., NAKAMURA F., KONG S., ARCE H.G., CARPENTER J.M., OSSENKOPF-OKADA V., KLESSEN R., SANHUEZA P., SHIMAJIRI Y., TSUKAGOSHI T., KAWABE R., ISHII S., DOBASHI K., SHIMOIKURA T., GOLDSMITH P.F., SANCHEZ-MONGE A., KAUFFMANN J., PILLAI T.G.S., PADOAN P., GINSBERG A., SMITH R.J., BALLY J., MAIRS S., PINEDA J.E., LIS D.C., BURKHART B., SCHILKE P., CHEN H.H.-H., ISELLA A., FRIESEN R.K., GOODMAN A.A. and HARPER D.A.
Abstract (from CDS):
Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.
Journal keyword(s): Star formation - Interstellar medium - Molecular clouds - Protostars - Radio observatories - CO line emission - Initial mass function
Simbad objects: 12
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