The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Bodo L. Ziegler sits on this spectrum.
This scientist: 335 publications — 24th percentile
24% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Bodo L. Ziegler sits on this spectrum.
This scientist: 76 D-Index — 11th percentile
11% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
His primary areas of study are Astrophysics, Galaxy, Redshift, Astronomy and Stellar mass. His studies in Star formation, Metallicity, Hubble Deep Field, Galaxy formation and evolution and Spiral galaxy are all subfields of Astrophysics research. As a member of one scientific family, Bodo L. Ziegler mostly works in the field of Galaxy, focusing on Stars and, on occasion, Photoionization.
Bodo L. Ziegler has included themes like Spectroscopy and Wavelength in his Redshift study. As a part of the same scientific study, Bodo L. Ziegler usually deals with the Lenticular galaxy, concentrating on Galaxy group and frequently concerns with Disc, Galaxy merger and Bulge. His Stellar population research incorporates elements of Stellar evolution and Surface brightness.
His primary areas of investigation include Astrophysics, Galaxy, Astronomy, Redshift and Elliptical galaxy. His work in Star formation, Galaxy cluster, Galaxy formation and evolution, Spiral galaxy and Lenticular galaxy is related to Astrophysics. Galaxy is a component of his Galaxy rotation curve, Metallicity, Luminosity, Stellar population and Stellar mass studies.
Brightest cluster galaxy, Luminous infrared galaxy, Galaxy group, Galaxy merger and Disc are among the areas of Astronomy where the researcher is concentrating his efforts. His work on Hubble Deep Field is typically connected to Field as part of general Redshift study, connecting several disciplines of science. The concepts of his Elliptical galaxy study are interwoven with issues in Radio galaxy and Bulge.
Bodo L. Ziegler focuses on Astrophysics, Galaxy, Star formation, Redshift and Stellar mass. His research on Astrophysics frequently connects to adjacent areas such as Astronomy. His work on Luminous infrared galaxy, Brightest cluster galaxy, Elliptical galaxy and Type-cD galaxy as part of his general Astronomy study is frequently connected to Instability, thereby bridging the divide between different branches of science.
His research in Star formation intersects with topics in Spatially resolved, Intracluster medium and Active galactic nucleus. His work deals with themes such as COSMIC cancer database, Radius, Emission spectrum and Supernova, which intersect with Redshift. His Galaxy formation and evolution study combines topics in areas such as Subgiant and Mass segregation.
Bodo L. Ziegler mostly deals with Astrophysics, Galaxy, Galaxy cluster, Star formation and Astronomy. His study in Bulge, Redshift, Galaxy formation and evolution and Mass distribution is carried out as part of his studies in Astrophysics. He applies his multidisciplinary studies on Galaxy and Kinematics in his research.
His research in Star formation intersects with topics in Field spectroscopy, Spatially resolved and Metallicity. His research in Astronomy is mostly focused on Brightest cluster galaxy. His work in Brightest cluster galaxy tackles topics such as Galaxy group which are related to areas like Disc, Galaxy merger and Galaxy groups and clusters.
S. F. Sánchez;R. C. Kennicutt;A. Gil de Paz;G. van de Ven
R. A. Marino;F. F. Rosales-Ortega;S. F. Sánchez;A. Gil de Paz
R. A. Marino;F. F. Rosales-Ortega;F. F. Rosales-Ortega;Sebastian Francisco Sanchez Sanchez;A. Gil De Paz
S. F. Sanchez;F. F. Rosales-Ortega;B. Jungwiert;J. Iglesias-Paramo
R. Singh;G. van de Ven;K. Jahnke;M. Lyubenova
S. F. Sanchez;R. C. Kennicutt;A. Gil de Paz;G. van de Ven
S. F. Sánchez;R. García-Benito;S. Zibetti;C. J. Walcher
C. J. Walcher;L. Wisotzki;S. Bekeraité;B. Husemann;B. Husemann
R. Singh;G. van de Ven;K. Jahnke;M. Lyubenova
A. Biviano;P. Rosati;I. Balestra;A. Mercurio
S. F. Sánchez;S. F. Sánchez;F. F. Rosales-Ortega;B. Jungwiert;J. Iglesias-Páramo
A. Gabasch;U. Hopp;G. Feulner;R. Bender
A. Bohm;B. L. Ziegler;R. P. Saglia;R. Bender
W. Kapferer;C. Sluka;S. Schindler;C. Ferrari
A. Biviano;P. Rosati;I. Balestra;A. Mercurio
C. Maier;C. Maier;S. J. Lilly;B. L. Ziegler;T. Contini;T. Contini
Ralf Bender;R. P. Saglia;Bodo Ziegler;Paola Belloni
A. Boehm;B.L. Ziegler;R.P. Saglia;R. Bender
Ralf Bender;Bodo Ziegler;Gustavo Bruzual
R. Bender;R. P. Saglia;B. Ziegler;P. Belloni
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