Auf dieser Seite finden sie einige Programme, die von Mitgliedern des Instituts entwickelt wurden. Die Programme können zu wissenschaftlichen Zwecken genutzt werden. Die Lizenzbedingungen finden Sie in den jeweiligen README-Dateien der Programmpakete.
GalIMF version 1.0.0
by Yan Zhiqiang
Description
GalIMF stands for the Galaxy-wide Initial Mass Function. It is a Python 3 module that allows users to compute galaxy-wide initial stellar mass functions based on locally derived empirical constraints following the IGIMF theory. See GalIMF homepage for more information.
| 191 K |
McLuster
von Andreas Küpper
Beschreibung
McLuster is a tool to make a star cluster. The code generates a table of cluster stars which can also be used as input for Nbody codes.
Online Dokumentation: http://www.astro.uni-bonn.de/~akuepper/mcluster/mcluster.html
Eine aktuelle Version ist ebenfalls zu finden unter http://www.astro.uni-bonn.de/~akuepper/mcluster/mcluster.html
| 283 K |
optimal_sampling
von Jan Pflamm-Altenburg
Beschreibung
The routine optimal_sampling allows to draw stellar masses from an IMF such that the IMF is optimally sampled without stochastic fluctuations.../../~akuepper/mcluster/mcluster.html
bhint
von Ulf Löckmann
Beschreibung
bhint is a post-Newtonian, high-precision integrator for stellar systems surrounding a super-massive black hole.
Weitere Informationen
Löckmann, U., & Baumgardt, H. 2008 MNRAS, 384, 32
"Tracing intermediate-mass black holes in the Galactic Centre"
| 240 K |
statpl
von Thomas Maschberger
Beschreibung
statpl is a program which estimates the parameter of power-law distributed data and calculates goodness-of-fit tests for them.
Weitere Informationen
Thomas Maschberger & Pavel Kroupa, 2009, MNRAS, accepted
"Estimators for the exponent and upper limit, and goodness-of-fit tests for (truncated) power-law distributions"
| 130 K |
Plumix
von Ladislav Subr
Beschreibung
Plumix is a small package for generating mass segregated star clusters. Its output can be directly used as input initial conditions for NBODY4 or NBODY6 code
Weitere Informationen
Subr, Kroupa & Baumgardt, 2008, MNRAS accepted; astro-ph/0801.2768
"A new method to create initially mass segregated star clusters in virial equilibrium"
| 6.8 K |
mkj_libs
von Manuel Metz
Beschreibung
mkj_libs provides a set of helper routines (vector operations, astrometry, statistical analysis of spherical data) for the main plane-fitting and analysis tools.
Online Dokumentation: http://www.astro.uni-bonn.de/~mmetz/py/docs/mkj_libs/index.html
Weitere Informationen
Metz, M.; Kroupa, P. & Jerjen, H., 2007, MNRAS, 374, 1125
"The spatial distribution of the Milky Way and Andromeda satellite galaxies"
| 17.7 K |
Libimf
von Jan Pflamm-Altenburg
Beschreibung
Libimf provides a collection of programming functions based on the general IMF-algorithm by Pflamm-Altenburg & Kroupa (2006).
Weitere Informationen
Pflamm-Altenburg, J. & Kroupa, P., 2006, MNRAS, accepted
"A highly abnormal massive-star mass function in the Orion Nebula cluster and the dynamical decay of trapezia systems"
| 10.7 K |
Catena
von Jan Pflamm-Altenburg
Beschreibung
Catena integrates the orbits of an ensemble of stars using the chain-regularization method (Mikkola & Aarseth) with an embedded Runge-Kutta integration method of 9(8)th order (Prince & Dormand).
Weitere Informationen
Pflamm-Altenburg, J. & Kroupa, P., 2006, MNRAS, accepted
"A highly abnormal massive-star mass function in the Orion Nebula cluster and the dynamical decay of trapezia systems"