Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations-Reference-Cited by-同舟云学术

Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations

Published:2018-10-26 Issue:1 Volume:482 Page:384-401
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Xiao Lin¹²³^ORCID,Galbany L⁴,Eldridge J J³^ORCID,Stanway Elizabeth R⁵^ORCID

Affiliation:

1. CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, 230026, China

2. School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei 230026, China

3. Department of Physics, University of Auckland, NZ

4. PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA

5. Department of Physics, University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL

Funder

National Key R&D Programme of China

National Natural Science Foundation of China

National Science Foundation

University of Auckland

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/1/384/26179081/sty2557.pdf

Reference60 articles.

1. Erratum - Classification Parameters for the Emission-Line Spectra of Extragalactic Objects

2. Spatially Resolved MaNGA Observations of the Host Galaxy of Superluminous Supernova 2017egm

3. On the association between core-collapse supernovae and H ii regions

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