A highly abnormal massive star mass function in the Orion Nebula cluster and the dynamical decay of trapezium systems
Open Access
- 21 November 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 373 (1) , 295-304
- https://doi.org/10.1111/j.1365-2966.2006.11028.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 30 references indexed in Scilit:
- An upper limit to the masses of starsNature, 2005
- Statistical Confirmation of a Stellar Upper Mass LimitThe Astrophysical Journal, 2005
- The Palomar/MSU Nearby Star Spectroscopic Survey. IV. The Luminosity Function in the Solar Neighborhood and M Dwarf KinematicsThe Astronomical Journal, 2002
- Early type stars at high galactic latitudesAstronomy & Astrophysics, 2001
- The Origin of Runaway StarsThe Astrophysical Journal, 2000
- From NBODY1 to NBODY6: The Growth of an IndustryPublications of the Astronomical Society of the Pacific, 1999
- Mass segregation in young stellar clustersMonthly Notices of the Royal Astronomical Society, 1998
- On the Stellar Population and Star-Forming History of the Orion Nebula ClusterThe Astronomical Journal, 1997
- On the Exponential Instability of N-Body SystemsThe Astrophysical Journal, 1993
- The velocity dispersion of the Orion Nebula cluster.The Astronomical Journal, 1988