Hostname: page-component-7bb8b95d7b-l4ctd Total loading time: 0 Render date: 2024-09-16T09:40:42.323Z Has data issue: false hasContentIssue false
  • English
  • Français

GalevNB: from simulations to observations

Published online by Cambridge University Press:  31 March 2017

Xiaoying Pang ,
Christoph Olczak  and
Rainer Spurzem
Xiaoying Pang
Affiliation:
Shanghai Institute of Technology, 100 Haiquan Road, Fengxian district, Shanghai 201418, P.R. China email: [email protected] National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
Christoph Olczak
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
Rainer Spurzem
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present GalevNB (Galev for N-body simulations), an utility that converts fundamental stellar properties of N-body simulations into observational properties using the GALEV (GAlaxy EVolutionary synthesis models) package, and thus allowing direct comparisons between observations and N-body simulations. It converts the fundamental stellar properties of N-body simulations, i.e., stellar mass, temperature, stellar luminosity and metallicity, into observational magnitudes for a variety of filters of widely used instruments/telescopes (HST, ESO, SDSS, 2MASS), and into spectra that span from far-UV (90 Å) to near-IR (160 μm).

Keywords

N-bodymagnitudespectra
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 259 - 260
Copyright
Copyright © International Astronomical Union 2017 

References

Aarseth, S. J. 1999, PASP, 111, 1333 Google Scholar
Kotulla, R., Fritze, U., Weilbacher, P., & Anders, P. 2009, MNRAS, 396, 462 Google Scholar
Lejeune, T., Cuisinier, F., & Buser, R. 1997, A&A Supplement, 125, 229 Google Scholar
Lejeune, T., Cuisinier, F., & Buser, R. 1998, A&A Supplement, 130, 65 Google Scholar