Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-26T11:45:00.625Z Has data issue: false hasContentIssue false
  • English
  • Français

Binary interactions and SFR calibrations

Published online by Cambridge University Press:  21 March 2013

Fenghui Zhang ,
Lifang Li  and
Zhanwen Han
Fenghui Zhang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming, 650011, China Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming, China email: [email protected]
Lifang Li
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming, 650011, China Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming, China email: [email protected]
Zhanwen Han
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming, 650011, China Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming, China email: [email protected]
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 discuss the effect of binary interactions on the tracers of star formation rate (including L1500, L2800, LHα, L[OII] and LFIR) at different metallicities (0.0001–0.03).

Keywords

binaries: general — galaxies: fundamental parameters — galaxies: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 340
Copyright
Copyright © International Astronomical Union 2013

References

Zhang, F., Li, L., Han, Z., Kang, X., & Zhuang, Y. 2012, MNRAS, submittedGoogle Scholar