9315455 Phinney Several related studies in theoretical astrophysics will be conducted. One concerns interactions between members of binary star systems which are caused by the fact that stars are neither static nor elastic. Mass transfer between an ordinary star and its black hole or neutron star companion will be modeled to account for observations of x-ray binaries and planets orbiting pulsars. A broad research program will be undertaken which is aimed at understanding how stars may form in the densest nuclei of galaxies and what these stars tell us about star formation. ***

Agency
National Science Foundation (NSF)
Institute
Division of Astronomical Sciences (AST)
Application #
9315455
Program Officer
Eileen D. Friel
Project Start
Project End
Budget Start
1994-03-15
Budget End
1997-08-31
Support Year
Fiscal Year
1993
Total Cost
$159,200
Indirect Cost
Name
California Institute of Technology
Department
Type
DUNS #
City
Pasadena
State
CA
Country
United States
Zip Code
91125