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.
Advection-dominated accretion: A self-similar solution
Countries citing papers authored by Ramesh Narayan
Since
Specialization
Citations
This map shows the geographic impact of Ramesh Narayan'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 Ramesh Narayan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Ramesh Narayan more than expected).
This network shows the impact of papers produced by Ramesh Narayan. 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 Ramesh Narayan. The network helps show where Ramesh Narayan may publish in the future.
Co-authorship network of co-authors of Ramesh Narayan
This figure shows the co-authorship network connecting the top 25 collaborators of Ramesh Narayan.
A scholar is included among the top collaborators of Ramesh Narayan 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 Ramesh Narayan. Ramesh Narayan is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Chael, Andrew, Katherine L. Bouman, Michael D. Johnson, et al.. (2019). ehtim: Imaging, analysis, and simulation software for radio interferometry. Astrophysics Source Code Library.2 indexed citations
Hjellming, R. M., M. P. Rupen, A. J. Mioduszewski, & Ramesh Narayan. (2000). Enhanced Radio Activity in the Quiescent State of the X-ray Transient V404 Cyg (=GS2023+338). ATel. 54. 1.1 indexed citations
Narayan, Ramesh & Tsvi Piran. (1996). Cooling Time Scales and Temporal Structure of Gamma-Ray Bursts. CERN Bulletin.140 indexed citations
16.
Narayan, Ramesh, Rohan Mahadevan, & Insu Yi. (1994). Advection dominated accretion model for sagittarius A: Evidence for a 10**6 solar mass black hole at the galactic center. Nature.
17.
Narayan, Ramesh, et al.. (1993). Magnification bias and gravitational lensing statistics. 31. 217.1 indexed citations
18.
Narayan, Ramesh & B.S. Sheshadri. (1992). Kinetics and morphological studies of silver cementation on copper single crystals in acidic medium. 30(1). 19–24.2 indexed citations
19.
Narayan, Ramesh. (1992). The physics of pulsar scintillation. Philosophical Transactions of the Royal Society of London Series A Physical and Engineering Sciences. 341(1660). 151–165.137 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.