What is he best known for?
The fields of study he is best known for:
- Galaxy
- Astronomy
- Milky Way
His main research concerns Astrophysics, Galaxy, Astronomy, Star formation and Stellar mass.
His Lenticular galaxy, Elliptical galaxy, Schwarzschild radius, Surface brightness and Stellar population investigations are all subjects of Astrophysics research.
G. van de Ven combines subjects such as Stellar kinematics, Angular momentum and Photometry with his study of Lenticular galaxy.
His work on Redshift, Galaxy formation and evolution, Metallicity and Active galactic nucleus as part of general Galaxy research is frequently linked to Abundance, thereby connecting diverse disciplines of science.
His Peculiar galaxy and Galaxy merger study are his primary interests in Astronomy.
The Star formation study combines topics in areas such as Early type and Disc galaxy.
His most cited work include:
- The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies (955 citations)
- CALIFA, the Calar Alto Legacy Integral Field Area survey : I. Survey presentation (886 citations)
- The SAURON project -- X. The orbital anisotropy of elliptical and lenticular galaxies: revisiting the (V/sigma,epsilon) diagram with integral-field stellar kinematics (456 citations)
What are the main themes of his work throughout his whole career to date?
G. van de Ven mostly deals with Astrophysics, Galaxy, Astronomy, Star formation and Stars.
His studies in Metallicity, Elliptical galaxy, Stellar population, Velocity dispersion and Globular cluster are all subfields of Astrophysics research.
The various areas that G. van de Ven examines in his Velocity dispersion study include Fundamental plane and Rotation.
The study of Galaxy is intertwined with the study of Kinematics in a number of ways.
His research in Star formation intersects with topics in Early type and Supermassive black hole.
His Surface brightness research incorporates themes from Position angle, Luminosity and Schwarzschild radius.
He most often published in these fields:
- Astrophysics (95.11%)
- Galaxy (76.69%)
- Astronomy (40.23%)
What were the highlights of his more recent work (between 2017-2021)?
- Astrophysics (95.11%)
- Galaxy (76.69%)
- Fornax Cluster (11.65%)
In recent papers he was focusing on the following fields of study:
His scientific interests lie mostly in Astrophysics, Galaxy, Fornax Cluster, Metallicity and Globular cluster.
All of his Astrophysics and Stellar population, Star formation, Stars, Accretion and Velocity dispersion investigations are sub-components of the entire Astrophysics study.
Astronomy covers G. van de Ven research in Galaxy.
His Fornax Cluster study incorporates themes from VLT Survey Telescope, Halo and Virial theorem.
The concepts of his Metallicity study are interwoven with issues in Multi Unit Spectroscopic Explorer and Stellar kinematics.
G. van de Ven has included themes like Galaxy formation and evolution, Planetary nebula and Star cluster in his Globular cluster study.
Between 2017 and 2021, his most popular works were:
- The Fornax 3D project: unveiling the thick disk origin in FCC 170: signs of accretion? (42 citations)
- Fornax3D project: Overall goals, galaxy sample, MUSE data analysis, and initial results (42 citations)
- The Fornax 3D project: Unveiling the thick disk origin in FCC 170; possible signs of accretion (42 citations)
In his most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Milky Way
G. van de Ven mainly investigates Galaxy, Astrophysics, Fornax Cluster, Globular cluster and Metallicity.
His study connects Spectrograph and Galaxy.
His Astrophysics study frequently links to other fields, such as Moment.
As a part of the same scientific family, G. van de Ven mostly works in the field of Fornax Cluster, focusing on Radius and, on occasion, Virial theorem.
As part of one scientific family, G. van de Ven deals mainly with the area of Globular cluster, narrowing it down to issues related to the Planetary nebula, and often Velocity dispersion and Radial velocity.
His Metallicity study combines topics from a wide range of disciplines, such as Star formation, Multi Unit Spectroscopic Explorer and Stellar kinematics.
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