M. Scholz

发表

Dynamical opacity-sampling models of Mira variables – II. Time-dependent atmospheric structure and observable properties of four M-type model series

Michael J. Ireland, Michael Scholz, M. Ireland, 2011, 1107.3619.

Molecular opacities in m - star atmospheres

F. Allard, R. Wehrse, M. Scholz, 1992 .

On the atmospheric structure and fundamental parameters of red supergiants

F. J. Abellán, P. Hauschildt, P. Wood, 2014, Proceedings of the International Astronomical Union.

Inhomogeneities in molecular layers of Mira atmospheres

M. Ireland, K. Ohnaka, A. Zijlstra, 2011, 1107.0842.

The K-Band Intensity Profile of R Leonis Probed by VLTI/VINCI

S. Ciroi, P. Wood, F. Paresce, 2008 .

The K-band intensity profile of R Leonis probed by VLTI/VINCI ⋆

Astrophysics, S. O. Physics, U. Padova, 2004, astro-ph/0411133.

On the interpretation of stellar disc observations in terms of diameters

M. Scholz, 2001 .

The K-band intensity profile of R Leonis probed by VLTI/VINCI ⋆

Astrophysics, S. O. Physics, U. Padova, 2004, astro-ph/0411133.

Pulsation of M-type Mira variables with moderately different mass: search for observable mass effects

P. Tuthill, M. Ireland, P. Wood, 2004, astro-ph/0408540.

Monochromatic Radii: A Tool of Mira Diagnostics

M. Scholz, 2003 .

Optical and near-IR spectra of O-rich Mira variables: A comparison between models and observations

P. Wood, A. Lançon, A. Tej, 2003, astro-ph/0309689.

Molecular and Dusty Layers of Asymptotic Giant Branch Stars Studied with the VLT Interferometer

M. Ireland, K. Ohnaka, A. Zijlstra, 2011 .

Comparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observations

K. Ohnaka, P. Wood, M. Scholz, 2005, astro-ph/0510214.

Silicate condensation in Mira variables

H. Gail, A. Pucci, M. Scholz, 2016, 1604.04636.

Dynamical opacity-sampling models of Mira variables - I. Modelling description and analysis of approximations

M. Ireland, P. Wood, M. Scholz, 2008, 0810.0560.

Pulsation of M-type Mira variables with moderately different mass: search for observable mass effects

P. Tuthill, M. Ireland, P. Wood, 2004, astro-ph/0408540.

The Influence of Atmospheric Dust on Limb Darkening of M-type Mira Variables

T. Bedding, P. Wood, M. Scholz, 2001 .

Observable effects of dust formation in dynamic atmospheres of M-type Mira variables

M. Scholz, M. Ireland, M. J. Ireland, 2006, astro-ph/0601383.

Abundances in intermediate-mass AGB stars undergoing third dredge-up and hot-bottom burning

J. Lattanzio, P. Wood, K. Hinkle, 2007, 0704.1907.

Optical and near-IR spectra of O-rich Mira variables: A comparison between models and observations

P. Wood, A. Lançon, A. Tej, 2003, astro-ph/0309689.

The structure of H2O shells in Mira atmospheres Correlation with disk brightness distributions and a spectrophotometric signature

A. Lançon, A. Tej, M. Scholz, 2003 .

Effects of moderate abundance changes on the atmospheric structure and colours of Mira variables

M. Ireland, P. Wood, M. Scholz, 2014, 1404.6735.

2 3 Se p 20 04 Mira science with interferometry : a review

M. Scholz, 2004 .

Wavelength dependence of angular diameters of M giants: an observational perspective

T. Bedding, J. Robertson, A. Jacob, 1999, astro-ph/9911076.

Comparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observations

K. Ohnaka, P. Wood, M. Scholz, 2005, astro-ph/0510214.

Extended static stellar atmospheres – V. Photospheres of luminous M stars

R. Wehrse, J. Schmid-Burgk, M. Scholz, 1981 .

Multi-wavelength bispectrum speckle interferometry of R Cas and comparison of the observations with Mira star models

G. Weigelt, Y. Balega, K. Hofmann, 2000 .

The Mira star S Ori: SiO maser shells related to the stellar photosphere, the molecular layers, and the dust shell at three epochs

K. Ohnaka, T. Driebe, D. Boboltz, 2007, Proceedings of the International Astronomical Union.

Opacity Problems in Cool Low Mass Stars

R. Wehrse, M. Scholz, 1994 .

On the possibility of formation of dust grains in M-type photospheres

J. Schmid-Burgk, M. Scholz, 1981 .

On the observability of geometric pulsation of M-type Mira variables

M. Ireland, P. Wood, M. Scholz, 2004 .

The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs

M. Wittkowski, M. Scholz, K. Ohnaka, 2007, 0705.4614.

SiO maser emission in Miras

M. Wittkowski, M. Scholz, D. Boboltz, 2008, 0811.2770.

Element abundances in O- and early B-stars

M. Scholz, 1972 .

Mira science with interferometry: a review

Michael Scholz, M. Scholz, 2003, SPIE Astronomical Telescopes + Instrumentation.

An Observational Test of the Spherical Model Atmospheres for the M Class Giants: The Case of δ2 Lyrae

H. M. Dyck, J. Benson, J. Sudol, 2002 .

Dust-driven winds of AGB stars : The critical interplay of atmospheric shocks and luminosity variations

N. T. Thao, Dimitri, H. Gail, 2016 .

THE KECK APERTURE MASKING EXPERIMENT: SPECTRO-INTERFEROMETRY OF THREE MIRA VARIABLES FROM 1.1 TO 3.8 μm

W. C. Danchi, T. R. Bedding, J. D. Monnier, 2008, 0811.1642.

Effects of molecular contamination of IR near‐continuum bandpasses on measurements of M‐type Mira diameters

A. Jacob, M. Scholz, 2002 .

New diameter measurements of 10 Mira Variables: implications for effective temperatures, atmospheric structure and pulsation modes

Peter G. Tuthill, Christopher A. Haniff, Michael Scholz, 1995 .

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

F. J. Abellán, P. Hauschildt, P. Wood, 2015, 1501.01560.

Extended static stellar atmospheres – VI. Search for a three-dimensional classification scheme for luminous M stars

R. Wehrse, M. Scholz, 1982 .