Theoretical evolution of optical strong lines across cosmic time

Kewley, Lisa; Dopita, Michael; Leitherer, Claus; Dave, Romeel; Yuan, T.-T.; Allen, Mark G.; Groves, Brent A; Sutherland, Ralph

Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Theoretical evolution of optical strong lines across cosmic time

Date

2013

Authors

Kewley, Lisa

Dopita, Michael

Leitherer, Claus

Dave, Romeel

Yuan, T.-T.

Allen, Mark G.

Groves, Brent A

Sutherland, Ralph

Publisher

IOP Publishing

Abstract

We use the chemical evolution predictions of cosmological hydrodynamic simulations with our latest theoretical stellar population synthesis, photoionization, and shock models to predict the strong line evolution of ensembles of galaxies from z = 3 to the

URI

http://hdl.handle.net/1885/73839

Collections

Open Access Research

Source

Astrophysical Journal, The

Type

Journal article

DOI

10.1088/0004-637X/774/2/100

Restricted until

2037-12-31

Downloads

File

Description

01_Kewley_Theoretical_evolution_of_2013.pdf (1.25 MB)

Full item page

Cultural advice

Theoretical evolution of optical strong lines across cosmic time

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

Keywords

Citation

URI

Collections

Source

Type

Book Title

Entity type

Access Statement

License Rights

DOI

Restricted until

Downloads