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.
The r-process and neutrino-heated supernova ejecta
1994497 citationsB. S. Meyer et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of B. S. Meyer'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 B. S. Meyer with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. S. Meyer more than expected).
This network shows the impact of papers produced by B. S. Meyer. 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 B. S. Meyer. The network helps show where B. S. Meyer may publish in the future.
Co-authorship network of co-authors of B. S. Meyer
This figure shows the co-authorship network connecting the top 25 collaborators of B. S. Meyer.
A scholar is included among the top collaborators of B. S. Meyer 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 B. S. Meyer. B. S. Meyer is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Meyer, B. S. & K. R. Bermingham. (2020). Exploding White Dwarf Stars and the Carriers of Nucleosynthetic Isotope Anomalies. Lunar and Planetary Science Conference. 2652.
6.
Dwarkadas, Vikram V., et al.. (2018). Triggered Star Formation at the Periphery of the Shell of a Wolf-Rayet Bubble as the Origin of the Solar System. LPI. 1304.3 indexed citations
7.
Meyer, B. S. & Justin Zhan. (2015). Drowning in opinions: Extracting the pearls. Journal of Computer Science & Systems Biology.3 indexed citations
8.
Meyer, B. S. & Donald D. Clayton. (2015). Sizes of Carbon Grains Condensing in SNII Shells. 78(1856). 5318.1 indexed citations
9.
Meyer, B. S., et al.. (2013). Sensitivity of Nitrogen-15 Production in Explosive Helium Burning to Supernova Energies and Reaction Rates and Importance for Low-Density Supernova Graphite Grains. LPI. 3006.1 indexed citations
10.
Meyer, B. S., et al.. (2011). Production of Nitrogen-15 in Explosive Helium Burning and Supernova Presolar Grains. LPI. 2376.2 indexed citations
11.
Huss, G. R. & B. S. Meyer. (2009). Galactic Chemical Evolution and the Abundances of Short-lived Radionuclides Inherited by the Solar System from the Interstellar Medium. LPI. 1957.1 indexed citations
12.
Fedkin, A. V., et al.. (2009). Condensation in Supernova Ejecta at High Spatial Resolution. LPI. 1699.2 indexed citations
13.
Meyer, B. S., et al.. (2007). s-Process Branching at 186Re, the Abundance of 186Os, and Presolar Grains. LPI. 2055.3 indexed citations
14.
Quitté, G., A. N. Halliday, A. Markowski, et al.. (2006). Ni Isotopes in the Early Solar System: an Overview. AGUFM. 2006.1 indexed citations
15.
Meyer, B. S., D. D. Clayton, & M. F. El Eid. (2003). Injection of 182Hf into the Early Solar Nebula. LPI. 2074.1 indexed citations
16.
Meyer, B. S., et al.. (2001). Calculating Chemical Evolution on the Web. TigerPrints (Clemson University). 1785.3 indexed citations
17.
Meyer, B. S. & Donald D. Clayton. (1999). Molybdenum Isotopes from a Neutron Burst. TigerPrints (Clemson University). 1458.3 indexed citations
18.
Meyer, B. S., et al.. (1995). NSE is Not Necessarily a Good Guide to the Synthesis of 48Ca. Meteoritics and Planetary Science. 30(5). 548.2 indexed citations
19.
Harper, C. L., H. Wiesmann, L. E. Nyquist, et al.. (1991). Interpretation of the (super 50) Ti- (super 96) Zr anomaly correlation in CAI; NNSE Zr production limits and S/ R/ P decomposition of the bulk solar system zirconium abundances. 22. 517–518.4 indexed citations
20.
Howard, W. M., Donald D. Clayton, & B. S. Meyer. (1991). Xe-H and Ba-H from weak neutron burst. Meteoritics and Planetary Science. 26. 347.2 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.