Add to ORKGThesis. 1976. B.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Microfiche copy available in Archives and Science.Bibliography: leaves 34-35.B.S
A study of stellar chromospheres based on the internal structure of particular stars is presented. U...
In order to put strict observational constraints on the evolutionary status of the magnetic chemica...
I provide observational constraints on the size and period distribution of the Galactic cataclysmic ...
Throughout the domain of the H R diagram lie groupings of stars whose luminosity varies with time. T...
<p>We are working to understand how stars of different mass and composition evolve, and how stellar ...
The thesis is dealing with spectral analysis of the B[e] star FS CMa, a prototype of FS CMa stars gr...
Consideration of the many types of intrinsic variable stars, that is, those that pulsate, reveals th...
textThis dissertation describes a new detailed abundance study of field red horizontal branch star...
The β Cephei stars represent an important class of massive star pulsators that probe the evolution o...
Abstract. In this thesis I will introduce the evolutionary stages of Cataclysmic Variables (CVs) and...
The β Cephei stars represent an important class of massive star pulsators that probe the evolution o...
Color-Magnitude Diagrams (CMDs) are plots that compare the magnitudes (luminosities) of stars in dif...
A theoretical study of Population II variables has been carried out using the nonlinear approach and...
Stars in the night sky are not as quiet as they seem. A human being wandering on Earth few billions ...
A variable star is one which varies in brightness (or some other physical property). A graph of the ...
A study of stellar chromospheres based on the internal structure of particular stars is presented. U...
In order to put strict observational constraints on the evolutionary status of the magnetic chemica...
I provide observational constraints on the size and period distribution of the Galactic cataclysmic ...
Throughout the domain of the H R diagram lie groupings of stars whose luminosity varies with time. T...
<p>We are working to understand how stars of different mass and composition evolve, and how stellar ...
The thesis is dealing with spectral analysis of the B[e] star FS CMa, a prototype of FS CMa stars gr...
Consideration of the many types of intrinsic variable stars, that is, those that pulsate, reveals th...
textThis dissertation describes a new detailed abundance study of field red horizontal branch star...
The β Cephei stars represent an important class of massive star pulsators that probe the evolution o...
Abstract. In this thesis I will introduce the evolutionary stages of Cataclysmic Variables (CVs) and...
The β Cephei stars represent an important class of massive star pulsators that probe the evolution o...
Color-Magnitude Diagrams (CMDs) are plots that compare the magnitudes (luminosities) of stars in dif...
A theoretical study of Population II variables has been carried out using the nonlinear approach and...
Stars in the night sky are not as quiet as they seem. A human being wandering on Earth few billions ...
A variable star is one which varies in brightness (or some other physical property). A graph of the ...
A study of stellar chromospheres based on the internal structure of particular stars is presented. U...
In order to put strict observational constraints on the evolutionary status of the magnetic chemica...
I provide observational constraints on the size and period distribution of the Galactic cataclysmic ...