Ultraviolet spectra of extreme nearby star-forming regions – approaching a local reference sample for JWST

Ultraviolet spectra of extreme nearby star-forming regions – approaching a local reference sample for JWST

Nearby dwarf galaxies provide a unique laboratory in which to test stellar population models below Z(circle dot)/2. Such tests are particularly important for interpreting the surprising high-ionization ultraviolet (UV) line emission detected at z > 6 in recent years. We present HST/COS UV spectra...

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Bibliographic Details
Main Authors: Senchyna, Peter, Stark, Daniel P., Vidal-García, Alba, Chevallard, Jacopo, Charlot, Stéphane, Mainali, Ramesh, Jones, Tucker, Wofford, Aida, Feltre, Anna, Gutkin, Julia
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: OXFORD UNIV PRESS 2017
Subjects:
stars: massive
galaxies: evolution
galaxies: stellar content
ultraviolet: galaxies
Online Access:http://hdl.handle.net/10150/625962
http://arizona.openrepository.com/arizona/handle/10150/625962

Internet

http://hdl.handle.net/10150/625962
http://arizona.openrepository.com/arizona/handle/10150/625962

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