RR Lyrae stars with variable mean magnitudes

Documenti analoghi

• Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes
  di: Rathour, Rajeev Singh, et al.
  Pubblicazione: (2025)
• The Infrared Surface Brightness technique applied to RR Lyrae stars from the solar neighborhood
  di: Zgirski, Bartłomiej, et al.
  Pubblicazione: (2024)
• Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect
  di: Rathour, Rajeev Singh, et al.
  Pubblicazione: (2024)
• Distance to the Globular Cluster M 3 from the Infrared Surface Brightness Technique applied to RR Lyrae stars
  di: Zgirski, Bartłomiej, et al.
  Pubblicazione: (2025)
• The Baade-Wesselink projection factor of RR Lyrae stars -- Calibration from OHP/SOPHIE spectroscopy and Gaia DR3 parallaxes
  di: Bras, Garance, et al.
  Pubblicazione: (2024)