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The ionization parameter of star-forming galaxies evolves with the specific star formation rate

Abstract. We investigate the evolution of the ionization parameter of star-forming galaxies using a high-redshift (z∼ 1.5) sample from the FMOS-COSMOS (Fibre M

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Bibliographic Details
Main Authors: Kaasinen, Melanie (Author) , Kewley, Lisa (Author) , Bian, Fuyan (Author) , Groves, Brent (Author) , Kashino, Daichi (Author) , Silverman, John (Author) , Kartaltepe, Jeyhan (Author)
Format: Article (Journal)
Language:English
Published: 24 April 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 477, Issue: 4, Pages: 5568-5589
ISSN:1365-2966
DOI:10.1093/mnras/sty1012
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/sty1012
Verlag, Volltext: https://academic.oup.com/mnras/article/477/4/5568/4983132
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Author Notes:Melanie Kaasinen, Lisa Kewley, Fuyan Bian, Brent Groves, Daichi Kashino, John Silverman and Jeyhan Kartaltepe
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Summary:Abstract. We investigate the evolution of the ionization parameter of star-forming galaxies using a high-redshift (z∼ 1.5) sample from the FMOS-COSMOS (Fibre M
Item Description:Gesehen am 05.11.2019
In original form 2017 December 21
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty1012

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