Zeitabhängigkeit der Atmosphärenstruktur von M-Typ Mira-Variablen

Applicant Professor Dr. Michael Scholz

Subject Area Astrophysics and Astronomy

Term from 2004 to 2007

Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 5442250

Final Report Year 2007

Final Report Abstract

No abstract available

2005. Bull. AAS 37, p.1306. Precision imaging with adaptive optics aperture masking interferometry
Martinache F., Lloyd J.P., Tuthill P.G., Woodruff H.C., ten Brummelaar T.A., Turner N.H.
2006. A&A 446, 1119. Comparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observations
Ohnaka K., Scholz M., Wood P.R.
2006. Advances in Adaptive Optics II (eds Ellerbroek B.L., Bonaccini Calia D,), Proc. SPIE 6272, p.103. Sparse-aperture adaptive optics
Tuthill P.G., Lloyd J.P., Ireland M.J., Martinache F., Monnier J.D., Woodruff H.C., ten Brummelaar T.A., Turner N.H., Townes C.H.
2006. MNRAS 367, 1585. Observable effects of dust formation in dynamic atmospheres of M-type Mira variables
Ireland M.J., Scholz M.
2006. Stellar Pulsation and Evolution (eds Walker A.R., Bono G.), Mem. Soc. Astron. It. 77, 186. Imaging shock fronts in Mira atmospheres
Woodruff H.C., Lloyd J.P., ten Brummelaar T.A., Scholz M., Turner N.H., Tuthill P.G.
2007. A&A 470, 191. The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs
Wittkowski M., Boboltz D.A., Ohnaka K., Driebe T., Scholz M.
2007. MNRAS 378, 1089. Abundances in intermediate-mass AGB stars undergoing third dredge-up and hot-bottom burning
McSaveney J.A., Wood P.R., Scholz M., Lattanzio J.C., Hinkle K.H.