(5) Umn)

Identifiers

• name variant (5) Umn) 0.60 · backfill

Papers (1)

1. Pulsational pair instability as an explanation for the most luminous supernovae astro-ph · 2007 · author #11

Mentions

• 0710.3314 #11 · backfill · confidence 0.70 (5) Umn)

Frequent Coauthors

• 2 1 shared papers
• (2) ITEP 1 shared papers
• 3) 1 shared papers
• (3) MPA 1 shared papers
• 4 1 shared papers
• (4) LANL 1 shared papers
• 5) ((1) Ucsc 1 shared papers
• Alexander Heger (1 1 shared papers
• S. Blinnikov (1 1 shared papers
• S. E. Woosley (1) 1 shared papers