7 Einträge gefunden

1. 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, Peter

   2015 - Forschungsinformationssystem der UHH
2. VLTI/AMBER studies of the atmospheric structure and fundamental parameters of red giant and supergiant stars

   1. Arroyo-Torres, Belen
   2. Wittkowski, M.
   3. Marcaide, J. M.
   4. Abellan, F. J.
   5. Chiavassa, A
   6. Fabregat, J.
   7. Freytag, B.

   2015 - Forschungsinformationssystem der UHH
3. VLTI/AMBER observations of cold giant stars: atmospheric structures and fundamental parameters

   1. Arroyo-Torres, Belen
   2. Martí-Vidal, I.
   3. Marcaide, J.~M.
   4. Wittkowski, M.
   5. Guirado, J.~C.
   6. Hauschildt, Peter
   7. Quirrenbach, A.

   2014 - Forschungsinformationssystem der UHH - frei zugänglich
4. On the atmospheric structure and fundamental parameters of red supergiants

   1. Wittkowski, M.
   2. Arroyo-Torres, Belen
   3. Marcaide, J. M.
   4. Abellan, F. J.
   5. Chiavassa, A.
   6. Freytag, B.
   7. Scholz, M.

   2014 - Forschungsinformationssystem der UHH
5. The atmospheric structure and fundamental parameters of red supergiants

   1. Arroyo-Torres, B.
   2. Wittkowski, M.
   3. Marcaide, J.M.
   4. Hauschildt, Peter

   2013 - Forschungsinformationssystem der UHH
6. The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii

   1. Arroyo-Torres, Belen
   2. Wittkowski, M.
   3. Marcaide, J. M.
   4. Hauschildt, Peter H.

   2013 - Forschungsinformationssystem der UHH
7. Fundamental properties and atmospheric structure of the red supergiant VY Canis Majoris based on VLTI/AMBER spectro-interferometry

   1. Wittkowski, M.
   2. Hauschildt, Peter
   3. Arroyo-Torres, B.
   4. Marcaide, J.M.

   2012 - Forschungsinformationssystem der UHH