Add to ORKGThis NASA grant covers our ADP research program, which involved detailed radiative transfer calculations of hydrodynamic models of pulsating asymptotic giant branch stars. Synthetic spectra resulting from these calculations are compared with International Ultraviolet Explorer (IUE) observations of these stars to test the validity of the models
This is the author accepted manuscript. The final version is available from Oxford University Press ...
The demands of accurate predictions of radiative transfer for climate applications are well-document...
A radiation transfer model was modified to include semitransparent and opaque layers as well as mole...
An investigation of the atmospheric structure of non-Mira, asymptotic giant branch stars through NLT...
Dynamic atmosphere models of Mira-type stars, prepared using a code developed by G. H. Bowen, were a...
Some 40 publications that appeared in scientific journals from 1973 to 1981 as well as 45 scientific...
Context. Wind-driving in asymptotic giant branch (AGB) stars is commonly attributed to a two-step pr...
Propagation of pulsational waves through the atmosphere of the M supergiant alpha Ori was explored u...
Mira (o Ceti), the prototypical Mira variable, due to its proximity (D = 128⁺¹⁹₋₁₄ pc, van Leeuwen e...
A total of 61 well exposed low dispersion LWP observations were obtained from the brightest normal M...
Context. High angular resolution (sub)millimetre observations of asymptotic giant branch (AGB) stars...
Progress is reported in modeling cometary emission in the 18-cm OH transition with specific applicat...
Context. To properly understand the propagation of SiO masers within the shocked region of the circu...
Miras are fascinating stars. A kappa-mechanism in their atmosphere drives pulsations which produce c...
This grant, dating back more than 20 years has supported a variety of investigations of the chromosp...
This is the author accepted manuscript. The final version is available from Oxford University Press ...
The demands of accurate predictions of radiative transfer for climate applications are well-document...
A radiation transfer model was modified to include semitransparent and opaque layers as well as mole...
An investigation of the atmospheric structure of non-Mira, asymptotic giant branch stars through NLT...
Dynamic atmosphere models of Mira-type stars, prepared using a code developed by G. H. Bowen, were a...
Some 40 publications that appeared in scientific journals from 1973 to 1981 as well as 45 scientific...
Context. Wind-driving in asymptotic giant branch (AGB) stars is commonly attributed to a two-step pr...
Propagation of pulsational waves through the atmosphere of the M supergiant alpha Ori was explored u...
Mira (o Ceti), the prototypical Mira variable, due to its proximity (D = 128⁺¹⁹₋₁₄ pc, van Leeuwen e...
A total of 61 well exposed low dispersion LWP observations were obtained from the brightest normal M...
Context. High angular resolution (sub)millimetre observations of asymptotic giant branch (AGB) stars...
Progress is reported in modeling cometary emission in the 18-cm OH transition with specific applicat...
Context. To properly understand the propagation of SiO masers within the shocked region of the circu...
Miras are fascinating stars. A kappa-mechanism in their atmosphere drives pulsations which produce c...
This grant, dating back more than 20 years has supported a variety of investigations of the chromosp...
This is the author accepted manuscript. The final version is available from Oxford University Press ...
The demands of accurate predictions of radiative transfer for climate applications are well-document...
A radiation transfer model was modified to include semitransparent and opaque layers as well as mole...