What is he best known for?
The fields of study he is best known for:
- Astronomy
- Astrophysics
- Galaxy
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.
His most cited work include:
- Star Formation in Molecular Clouds: Observation and Theory (2009 citations)
- Self-similar collapse of isothermal spheres and star formation. (1483 citations)
- Magnetocentrifugally driven flows from young stars and disks. 1: A generalized model (1166 citations)
What are the main themes of his work throughout his whole career to date?
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.
He most often published in these fields:
- Astrophysics (67.11%)
- Astronomy (38.22%)
- Star formation (29.78%)
What were the highlights of his more recent work (between 2004-2016)?
- Astrophysics (67.11%)
- Accretion (17.33%)
- Star formation (29.78%)
In recent papers he was focusing on the following fields of study:
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.
Between 2004 and 2016, his most popular works were:
- Gravitational Collapse of Magnetized Clouds. I. Ideal Magnetohydrodynamic Accretion Flow (162 citations)
- Gravitational Collapse of Magnetized Clouds. I. Ideal Magnetohydrodynamic Accretion Flow (162 citations)
- Gravitational collapse of magnetized clouds. I. Ideal MHD accretion flow (160 citations)
In his most recent research, the most cited papers focused on:
- Astronomy
- Astrophysics
- Galaxy
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.
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