What causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres

  1. Arroyo-Torres, B.
  2. Wittkowski, M.
  3. Chiavassa, A.
  4. Scholz, M.
  5. Freytag, B.
  6. Marcaide, J.M.
  7. Hauschildt, P.H.
  8. Wood, P.R.
  9. Abellan, F.J.
Revista:
Astronomy and Astrophysics

ISSN: 1432-0746 0004-6361

Ano de publicación: 2015

Volume: 575

Tipo: Artigo

DOI: 10.1051/0004-6361/201425212 GOOGLE SCHOLAR lock_openAcceso aberto editor