2023 - Research.com Physics in Germany Leader Award
His scientific interests lie mostly in Astrophysics, Galaxy cluster, Astronomy, Galaxy and Cluster. Astrophysics is a component of his ROSAT, Redshift, Dark matter, Cooling flow and Planck studies. His study in Galaxy cluster is interdisciplinary in nature, drawing from both Luminosity, Radius and Velocity dispersion.
His work deals with themes such as Universe and Baryon, which intersect with Galaxy. His Cluster study combines topics from a wide range of disciplines, such as COSMIC cancer database, Mass-to-light ratio and Density contrast. His study looks at the relationship between Sky and topics such as Stars, which overlap with Quasar.
Astrophysics, Galaxy cluster, Galaxy, Astronomy and Cluster are his primary areas of study. His research in Redshift, ROSAT, Brightest cluster galaxy, Luminosity and Intracluster medium are components of Astrophysics. The ROSAT study combines topics in areas such as Redshift survey, Ecliptic pole and Flux.
His study explores the link between Galaxy cluster and topics such as Elliptical galaxy that cross with problems in Radio galaxy. Galaxy groups and clusters, Type-cD galaxy, Sky, Interacting galaxy and Abell 2744 are among the areas of Astronomy where the researcher is concentrating his efforts. His research integrates issues of Planck and Radius in his study of Cluster.
The scientist’s investigation covers issues in Astrophysics, Galaxy cluster, Astronomy, Galaxy and Cluster. All of his Astrophysics and Redshift, Planck, Luminosity, Brightest cluster galaxy and ROSAT investigations are sub-components of the entire Astrophysics study. As a member of one scientific family, Hans Böhringer mostly works in the field of Redshift, focusing on Sky and, on occasion, Supermassive black hole.
His Galaxy cluster research includes elements of Surface brightness and Velocity dispersion. In his study, which falls under the umbrella issue of Galaxy, Electron density is strongly linked to Spectral line. His Arcminute Microkelvin Imager study in the realm of Cluster interacts with subjects such as Scaling.
His primary scientific interests are in Astrophysics, Galaxy cluster, Astronomy, Galaxy and Planck. His Astrophysics study frequently draws connections to other fields, such as Cluster. His biological study spans a wide range of topics, including Observatory and Flux.
His work on Brightest cluster galaxy as part of general Galaxy cluster study is frequently linked to Context, bridging the gap between disciplines. Many of his studies involve connections with topics such as Dark matter and Galaxy. The study incorporates disciplines such as CMB cold spot, Baryon, Malmquist bias and Baryon acoustic oscillations in addition to Planck.
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.
Sloan Digital Sky Survey: Early data release
C. Stoughton;R. H. Lupton;M. Bernardi;M. R. Blanton.
web science (2002)
Sloan digital sky survey: Early data release
Chris Stoughton;Robert H. Lupton;Mariangela Bernardi;Michael R. Blanton;Michael R. Blanton.
The Astronomical Journal (2002)
Planck 2013 results. I. Overview of products and scientific results
P. A. R. Ade;N. Aghanim;M. I. R. Alves.
Astronomy and Astrophysics (2014)
The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
Thomas H. Reiprich;Hans Böhringer.
The Astrophysical Journal (2002)
The ROSAT Brightest Cluster Sample (BCS) - I. The compilation of the sample and the cluster log N-log S distribution
H. Ebeling;A.C. Edge;H. Böhringer;S.W. Allen.
arXiv: Astrophysics (1998)
The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y-SZ-M-500 relation
M. Arnaud;G. W. Pratt;R. Piffaretti;H. Böhringer.
Astronomy and Astrophysics (2010)
Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
P. A. R. Ade;N. Aghanim;M. Arnaud.
arXiv: Cosmology and Nongalactic Astrophysics (2015)
The ROSAT Brightest Cluster Sample — I. The compilation of the sample and the cluster log N—log S distribution
H. Ebeling;H. Ebeling;A. C. Edge;H. Böhringer;S. W. Allen.
Monthly Notices of the Royal Astronomical Society (1998)
Evolution of buoyant bubbles in M87
E. Churazov;E. Churazov;M. Brüggen;M. Brüggen;C. R. Kaiser;H. Böhringer.
The Astrophysical Journal (2001)
A New Radio-X-Ray Probe of Galaxy Cluster Magnetic Fields
T. E. Clarke;T. E. Clarke;P. P. Kronberg;Hans Böhringer.
The Astrophysical Journal (2001)
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