Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Stellar Structure and Evolution
1990968 citationsRudolf Kippenhahn et al.profile →
Stellar Structure and Evolution
2012794 citationsRudolf Kippenhahn et al.profile →
Citations per year, relative to Rudolf Kippenhahn Rudolf Kippenhahn (= 1×)
peers
William H. Julian
Countries citing papers authored by Rudolf Kippenhahn
Since
Specialization
Citations
This map shows the geographic impact of Rudolf Kippenhahn's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Rudolf Kippenhahn with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Rudolf Kippenhahn more than expected).
Fields of papers citing papers by Rudolf Kippenhahn
This network shows the impact of papers produced by Rudolf Kippenhahn. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Rudolf Kippenhahn. The network helps show where Rudolf Kippenhahn may publish in the future.
Co-authorship network of co-authors of Rudolf Kippenhahn
This figure shows the co-authorship network connecting the top 25 collaborators of Rudolf Kippenhahn.
A scholar is included among the top collaborators of Rudolf Kippenhahn based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with Rudolf Kippenhahn. Rudolf Kippenhahn is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Kippenhahn, Rudolf. (2004). Von allen guten Geistern verlassen. 43(9). 40–41.2 indexed citations
2.
Kippenhahn, Rudolf. (2003). Christian Doppler (1803-1853). Ein Genie hat Geburtstag. 42(11). 34–37.
3.
Kippenhahn, Rudolf. (1983). 100 Billion Suns: The Birth, Life, and Death of the Stars. Internet Archive (Internet Archive).1 indexed citations
4.
Kippenhahn, Rudolf, H. U. Schmidt, & H. C. Thomas. (1980). UBV photometry of HZ HER : the shape of the primary minimum.. 90. 54.2 indexed citations
5.
Kippenhahn, Rudolf, et al.. (1980). The time scale of thermohaline mixing in stars. 91. 175–180.10 indexed citations
6.
Kippenhahn, Rudolf & H. C. Thomas. (1979). HZ Herculis and the match paradox.. 75. 281–290.1 indexed citations
7.
Kippenhahn, Rudolf & H. C. Thomas. (1978). Accretion belts on white dwarfs.. A&A. 63. 265–272.3 indexed citations
Kippenhahn, Rudolf, et al.. (1977). The interaction of variable stars with their environment.26 indexed citations
12.
Kippenhahn, Rudolf, et al.. (1977). The interaction of variable stars with their environment : proceedings of the IAU-Colloquium no. 42, Bamberg, September 6-9, 1977. Medical Entomology and Zoology. 121.6 indexed citations
13.
Kippenhahn, Rudolf. (1974). Circulation and Mixing. Symposium - International Astronomical Union. 66. 20–40.2 indexed citations
Kippenhahn, Rudolf. (1963). Stars with Helium-rich cores. Max Planck Digital Library. 330–368.1 indexed citations
17.
Baker, N. H. & Rudolf Kippenhahn. (1962). The Pulsations of Models of δ Cephei Stars. With 17 Figures in the Text. 54. 114.2 indexed citations
18.
Baker, Nancy L. & Rudolf Kippenhahn. (1959). Untersuchungen über rotierende Sterne. III. Meridionale Zirkulation bei nichtstarrer Rotation. 48. 140.1 indexed citations
19.
Kippenhahn, Rudolf. (1959). 23. Meridional Circulations in the Hydrogen Convective Layer of the Sun. 9. 249–255.1 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.