This map shows the geographic impact of E. Müeller'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 E. Müeller with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. Müeller more than expected).
This network shows the impact of papers produced by E. Müeller. 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 E. Müeller. The network helps show where E. Müeller may publish in the future.
Co-authorship network of co-authors of E. Müeller
This figure shows the co-authorship network connecting the top 25 collaborators of E. Müeller.
A scholar is included among the top collaborators of E. Müeller 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 E. Müeller. E. Müeller 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.
Müeller, E., et al.. (1997). Dynamics and gravitational wave signature of axisymmetric rotational core collapse. 320(1). 209–227.82 indexed citations
Janka, Hans‐Thomas & E. Müeller. (1996). Neutrino heating, convection, and the mechanism of Type-II supernova explosions.. OpenGrey (Institut de l'Information Scientifique et Technique). 306(1). 167–198.70 indexed citations
Martı́, J., E. Müeller, & J. Ibáñez. (1994). Hydrodynamical simulations of relativistic jets. 281(1).14 indexed citations
6.
Janka, Hans‐Thomas & E. Müeller. (1994). Neutron star recoils from anisotropic supernovae.. OpenGrey (Institut de l'Information Scientifique et Technique). 290. 496.18 indexed citations
7.
Hashimoto, M., Yoshiharu Eriguchi, K. Arai, & E. Müeller. (1993). Self-gravitating and rotating hot toroids. 268(1). 131–136.3 indexed citations
8.
Steinmetz, Matthias & E. Müeller. (1993). On the capabilities and limits of smoothed particle hydrodynamics. 268(1). 391–410.27 indexed citations
9.
Müeller, E., B. Fryxell, & D. Arnett. (1991). Instability and clumping in SN 1987A. 251(2). 505–514.56 indexed citations
Schaêfer, G., et al.. (1991). Gravitational waves from the collapse of rotating stellar cores. 246(2). 417–440.39 indexed citations
12.
Müeller, E., et al.. (1989). Hydrodynamics of the interstellar gas in colliding galaxies. II: Non-central collisions. 216. 19–30.1 indexed citations
13.
Müeller, E.. (1986). Nuclear-reaction networks and stellar evolution codes - The coupling of composition changes and energy release in explosive nuclear burning. 162. 103–108.5 indexed citations
Müeller, E.. (1982). Gravitational radiation from collapsing rotating stellar cores. A&A. 114(1). 53–59.5 indexed citations
16.
Hillebrandt, W. & E. Müeller. (1981). Computer simulations of stellar collapse and shock wave propagation. 103(1). 147–153.5 indexed citations
17.
Müeller, E. & W. Hillebrandt. (1981). The collapse of rotating stellar cores. 103(2). 358–366.11 indexed citations
18.
Müeller, E., W. Hillebrandt, & M. Różyczka. (1980). Stellar collapse - Adiabatic hydrodynamics and shock wave propagation. 81(3). 288–292.7 indexed citations
19.
Müeller, E.. (1979). A magnetohydrodynamic supernova model. PhDT.
20.
Müeller, E.. (1977). Highlights of astronomy. Volume 4 - International Astronomical Union, General Assembly, 16th, Grenoble, France, August 24-September 2, 1976, Proceedings. Parts 1 & 2. 4. 1.1 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.