pith. sign in

Celestijnenlaan 200D

Identifiers

  • name variant Celestijnenlaan 200D 0.50 · backfill

Papers (2)

  1. Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star astro-ph.SR · 2018 · author #53
  2. When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic astro-ph.SR · 2018 · author #24

Mentions

No mention provenance yet.

Frequent Coauthors