pith. sign in

I. Hubeny (4)

Identifiers

  • name variant I. Hubeny (4) 0.60 · backfill

Papers (1)

  1. A possible solution to the Lyman/Balmer line problem in hot DA white dwarfs astro-ph.SR · 2014 · author #5

Mentions

  • 1410.0811 #5 · backfill · confidence 0.70 I. Hubeny (4)

Frequent Coauthors