Core-collapse supernovae in low-metallicity environments and future all-sky transient surveys

David Young, Stephen Smartt, Seppo Mattila, N.R. Tanvir, D. Bersier, K.C. Chambers, N. Kaiser, J.L. Tonry

Research output: Contribution to journalArticlepeer-review

29 Citations (Scopus)

Abstract

Aims. Massive stars in low-metallicity environments may produce exotic explosions such as long-duration gamma-ray bursts and pair-instability supernovae when they die as core-collapse supernovae (CCSNe). Such events are predicted to be relatively common in the early Universe during the first episodes of star-formation. To understand these distant explosions it is vital to study nearby CCSNe arising in low-metallicity environments to determine if the explosions have different characteristics to those studied locally in high-metallicity galaxies. Many of the nearby supernova searches concentrate their efforts on high star-formation rate galaxies, hence biasing the discoveries to metal rich regimes. Here we determine the feasibility of searching for these CCSNe in metal-poor dwarf galaxies using various survey strategies.
Original languageEnglish
Pages (from-to)359-375
Number of pages17
JournalAstronomy and Astrophysics
Volume489
Issue number1
DOIs
Publication statusPublished - Oct 2008

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Core-collapse supernovae in low-metallicity environments and future all-sky transient surveys'. Together they form a unique fingerprint.

Cite this