... Esta investigaciцЕn aparece publicada en la revista Astronomy and Astrophysics (БЂњThe Mira variable S Ori: Relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochsБЂќ, por M. Wittkowski et al.) ...
... Esta investigaciцЕn aparece publicada en la revista Astronomy and Astrophysics (БЂњThe Mira variable S Ori: Relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochsБЂќ, por M. Wittkowski et al.) ...
... However, measurements in the infrared - although more difficult to perform - result in a better estimate of the diameter of the underlying atmosphere (photosphere) of a star. ...
... As a consequence, they go regularly through large amplitude oscillations that create very rapid motions of its apparent surface (the photosphere) with velocities up to 30 km/s, or 108 000 km/h! While this remains to be established, there could be a link ...
... As a consequence, they go regularly through large amplitude oscillations that create very rapid motions of its apparent surface (the photosphere) with velocities up to 30 km/s, or 108 000 km/h! While this remains to be established, there could be a link ...
... As a consequence, they go regularly through large amplitude oscillations that create very rapid motions of its apparent surface (the photosphere) with velocities up to 30 km/s, or 108 000 km/h! While this remains to be established, there could be a link ...
... As a consequence, they go regularly through large amplitude oscillations that create very rapid motions of its apparent surface (the photosphere) with velocities up to 30 km/s, or 108 000 km/h! While this remains to be established, there could be a link ...