English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Although Type Ia supernovae have been heavily scrutinized due to their use inmaking cosmological distance estimates, we are still unable to definitivelyidentify the progenitors for the entire population. While answers have beenpresented for certain specific systems, a complete solution remains elusive. Wepresent observations of two supernova remnants (SNRs) in the Large MagellanicCloud, SNR 0505-67.9 and SNR 0509-68.7, for which we have identified the centerof the remnant and the 99.73% containment central region in which any companionstar left over after the supernova must be located. Both remnants have a numberof potential ex-companion stars near their centers; all possible single anddouble degenerate progenitor models remain viable for these two supernovae.Future observations may be able to identify the true ex-companions for bothremnants.

Investigation of the Progenitors of the Type Ia Supernovae Associated With the LMC Supernova Remnants 0505-67.9 and 0509-68.7