Add to ORKGThe method and results of the computation of the model atmospheres and spectral energy distributions of chemically peculiar stars, are discussed. The models are computed with a special consideration of the particular problems encountered when computing model atmospheres for M and C-giants, and of hydrogen deficient stars. We present some computed model atmospheres for Sakurai's object, giants of globular clusters, and C-giants
In Schaerer et al. (1995, Paper I) we have presented the first "combined stellar structure and atmos...
Context.Historically, stellar model atmospheres with scaled solar abundances (for all elements heavi...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
Author Institution: Astronomy Department, Indiana UniversityIn order to study the importance of mole...
As stars evolve, their surfaces may be altered by several different mechanisms. These introduce dist...
We calculated 240 model atmospheres of carbon giants of high carbon abundances (2800 ≤ Teff ≤ 3400 K...
This report contains an extensive series of model atmospheres for cool stars having a wide range in ...
We present a series of papers with the central theme of molecular band spectrum synthesis of cool s...
Author Institution: Niels Bohr InstitueThe light that reach us from distant star, pass through a ``l...
This report contains an extensive series of model atmospheres for cool stars having a wide range in ...
Stellar model atmospheres form the basis for any element abundance determination and hence are cruci...
We present a detailed calculation of model atmospheres for DA white dwarfs. Our atmosphere code solv...
Based on a grid of hydrostatic spherical COMARCS models for cool stars, we have calculated observabl...
Our ability to extract information from the spectra of stars depends on reliable models of stellar a...
We present Very Low Mass stellar models as computed including non-grey model atmospheres for selecte...
In Schaerer et al. (1995, Paper I) we have presented the first "combined stellar structure and atmos...
Context.Historically, stellar model atmospheres with scaled solar abundances (for all elements heavi...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
Author Institution: Astronomy Department, Indiana UniversityIn order to study the importance of mole...
As stars evolve, their surfaces may be altered by several different mechanisms. These introduce dist...
We calculated 240 model atmospheres of carbon giants of high carbon abundances (2800 ≤ Teff ≤ 3400 K...
This report contains an extensive series of model atmospheres for cool stars having a wide range in ...
We present a series of papers with the central theme of molecular band spectrum synthesis of cool s...
Author Institution: Niels Bohr InstitueThe light that reach us from distant star, pass through a ``l...
This report contains an extensive series of model atmospheres for cool stars having a wide range in ...
Stellar model atmospheres form the basis for any element abundance determination and hence are cruci...
We present a detailed calculation of model atmospheres for DA white dwarfs. Our atmosphere code solv...
Based on a grid of hydrostatic spherical COMARCS models for cool stars, we have calculated observabl...
Our ability to extract information from the spectra of stars depends on reliable models of stellar a...
We present Very Low Mass stellar models as computed including non-grey model atmospheres for selecte...
In Schaerer et al. (1995, Paper I) we have presented the first "combined stellar structure and atmos...
Context.Historically, stellar model atmospheres with scaled solar abundances (for all elements heavi...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...