2005 - Fellow, The World Academy of Sciences
2000 - Dannie Heineman Prize for Astrophysics, American Astronomical Society
1992 - Fellow of the American Academy of Arts and Sciences
1987 - Member of the National Academy of Sciences
1972 - Fellow of Alfred P. Sloan Foundation
The scientist’s investigation covers issues in Astrophysics, Astronomy, Star formation, Protostar and Young stellar object. Borrowing concepts from Thick disk, he weaves in ideas under Astrophysics. His study focuses on the intersection of Astronomy and fields such as Magnetosphere with connections in the field of Chondrule, Chondrite and Meteoroid.
Frank H. Shu has researched Star formation in several fields, including Gravitational collapse, Classical mechanics and Mechanics. His research in Mechanics intersects with topics in Magnetohydrodynamics and Molecular cloud. His Protostar study integrates concerns from other disciplines, such as Stellar evolution, Radius and Angular momentum.
Astrophysics, Astronomy, Star formation, Stars and Gravitational collapse are his primary areas of study. His study in Protostar, Accretion, T Tauri star, Molecular cloud and Young stellar object falls within the category of Astrophysics. His research integrates issues of Solar System and Magnetosphere in his study of T Tauri star.
His study in Star formation is interdisciplinary in nature, drawing from both Stellar mass loss and Magnetohydrodynamics. The various areas that Frank H. Shu examines in his Stars study include Light curve and Dimensionless quantity. His Gravitational collapse study incorporates themes from Magnetic flux, Mechanics, Lorentz force and Bonnor–Ebert mass.
Frank H. Shu spends much of his time researching Astrophysics, Accretion, Star formation, Magnetohydrodynamics and Gravitational collapse. His Astrophysics study frequently links to related topics such as Astronomy. His work carried out in the field of Accretion brings together such families of science as Angular momentum and Young stellar object.
His Star formation study combines topics from a wide range of disciplines, such as Beryllium, Cosmic ray, Solar System, Formation and evolution of the Solar System and Supernova. His Magnetohydrodynamics research is multidisciplinary, relying on both Mechanics, Interstellar medium, Classical mechanics and Molecular cloud. The concepts of his Gravitational collapse study are interwoven with issues in Magnetic flux, Protostar, Bonnor–Ebert mass and Magnetohydrodynamic drive.
His main research concerns Magnetohydrodynamics, Accretion, Astrophysics, Star formation and Gravitational collapse. Interstellar medium is closely connected to Mechanics in his research, which is encompassed under the umbrella topic of Magnetohydrodynamics. His Astrophysics research includes themes of Astronomy, Magnetosphere and Gas dynamics.
His Astronomy study combines topics in areas such as Field line and Magnetization. He combines subjects such as Cosmic ray, Solar System, Formation and evolution of the Solar System, Supernova and Irradiation with his study of Star formation. His Gravitational collapse research includes elements of Magnetic flux and Protostar.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Star Formation in Molecular Clouds: Observation and Theory
Frank H. Shu;Fred C. Adams;Susana Lizano.
Annual Review of Astronomy and Astrophysics (1987)
Self-similar collapse of isothermal spheres and star formation.
F. H. Shu.
The Astrophysical Journal (1977)
Magnetocentrifugally driven flows from young stars and disks. 1: A generalized model
Frank Shu;Joan Najita;Eve Charis Ostriker;Frank Wilkin.
The Astrophysical Journal (1994)
Spectral evolution of young stellar objects
Fred C. Adams;Charles J. Lada;Frank H. Shu.
The Astrophysical Journal (1987)
On the Spiral Structure of Disk Galaxies.
C. C. Lin;Frank H. Shu.
The Astrophysical Journal (1964)
Photoevaporation of Disks around Massive Stars and Application to Ultracompact H II Regions
David Hollenbach;Doug Johnstone;Susana Lizano;Frank Shu.
The Astrophysical Journal (1994)
Gas dynamics of semidetached binaries
S. H. Lubow;F. H. Shu.
The Astrophysical Journal (1975)
ON THE SPIRAL STRUCTURE OF DISK GALAXIES. III. COMPARISON WITH OBSERVATIONS.
C. C. Lin;C. Yuan;Frank H. Shu.
The Astrophysical Journal (1969)
Toward an Astrophysical Theory of Chondrites
Frank H. Shu;Hsien Shang;Typhoon Lee.
PLANETESIMAL FORMATION BY GRAVITATIONAL INSTABILITY
Andrew N. Youdin;Frank H. Shu;Frank H. Shu.
The Astrophysical Journal (2002)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below: