B. W. Murphy

1.8k total citations
23 papers, 1.3k citations indexed

About

B. W. Murphy is a scholar working on Astronomy and Astrophysics, Instrumentation and Cognitive Neuroscience. According to data from OpenAlex, B. W. Murphy has authored 23 papers receiving a total of 1.3k indexed citations (citations by other indexed papers that have themselves been cited), including 14 papers in Astronomy and Astrophysics, 5 papers in Instrumentation and 3 papers in Cognitive Neuroscience. Recurrent topics in B. W. Murphy's work include Stellar, planetary, and galactic studies (11 papers), Astrophysics and Star Formation Studies (6 papers) and Astronomy and Astrophysical Research (5 papers). B. W. Murphy is often cited by papers focused on Stellar, planetary, and galactic studies (11 papers), Astrophysics and Star Formation Studies (6 papers) and Astronomy and Astrophysical Research (5 papers). B. W. Murphy collaborates with scholars based in United States, Netherlands and Germany. B. W. Murphy's co-authors include Alan H. Lockwood, David S. Wack, H. N. Cohn, Mary Lou Coad, Richard Salvi, R. H. Durisen, P. M. Lugger, Jeffrey N. Cuzzi, Thomas C. Mahl and Robert D. Van Valin and has published in prestigious journals such as Nature, The Astrophysical Journal and Hepatology.

In The Last Decade

B. W. Murphy

22 papers receiving 1.2k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
B. W. Murphy United States	16	499	454	425	328	116	23	1.3k
Gordon E. Sarty Canada	20	491 1.0×	50 0.1×	63 0.1×	88 0.3×	191 1.6×	76	1.2k
Andreas Metz United States	36	562 1.1×	49 0.1×	56 0.1×	47 0.1×	75 0.6×	129	5.6k
Rajat M. Thomas Netherlands	20	672 1.3×	11 0.0×	719 1.7×	55 0.2×	92 0.8×	36	1.6k
Robert I. Reid United States	25	671 1.3×	29 0.1×	95 0.2×	209 0.6×	32 0.3×	94	1.9k
Leighton Barnden Australia	24	200 0.4×	129 0.3×	67 0.2×	66 0.2×	32 0.3×	61	1.4k
Silvia Tommasin Italy	17	178 0.4×	13 0.0×	192 0.5×	93 0.3×	20 0.2×	43	785
T. Hilger Germany	20	127 0.3×	32 0.1×	588 1.4×	76 0.2×	11 0.1×	42	1.4k
Richard D. E. Saunders United Kingdom	25	162 0.3×	25 0.1×	528 1.2×	40 0.1×	5 0.0×	80	1.7k
Natasha Leporé United States	26	832 1.7×	24 0.1×	38 0.1×	146 0.4×	201 1.7×	135	2.5k

Countries citing papers authored by B. W. Murphy

Since Specialization

Citations

This map shows the geographic impact of B. W. Murphy'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. W. Murphy with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. W. Murphy more than expected).

Fields of papers citing papers by B. W. Murphy

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by B. W. Murphy. 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. W. Murphy. The network helps show where B. W. Murphy may publish in the future.

Co-authorship network of co-authors of B. W. Murphy

This figure shows the co-authorship network connecting the top 25 collaborators of B. W. Murphy. A scholar is included among the top collaborators of B. W. Murphy 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. W. Murphy. B. W. Murphy is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Hrivnak, Bruce J., G. D. Henson, T. C. Hillwig, et al.. (2019). Variability in Proto-planetary Nebulae. VI. Multitelescope Light Curve Studies of Several Medium-bright (V = 13–15), Carbon-rich Objects. The Astronomical Journal. 159(1). 21–21. 2 indexed citations

Murphy, B. W., H. N. Cohn, & P. M. Lugger. (2011). FOKKER-PLANCK MODELS FOR M15 WITHOUT A CENTRAL BLACK HOLE: THE ROLE OF THE MASS FUNCTION. The Astrophysical Journal. 732(2). 67–67. 17 indexed citations

Drukier, G. A., et al.. (2007). The Global Kinematics of the Globular Cluster M92. The Astronomical Journal. 133(3). 1041–1057. 21 indexed citations

Murphy, B. W., et al.. (2004). Tracking User Interactions Within Visualizations. 215. 1 indexed citations

Benedict, Ralph H. B., Alan H. Lockwood, Janet L. Shucard, et al.. (1998). Functional neuroimaging of attention in the auditory modality. Neuroreport. 9(1). 121–126. 82 indexed citations

Jaeger, Jeri J., Alan H. Lockwood, Robert D. Van Valin, et al.. (1998). Sex differences in brain regions activated by grammatical and reading tasks. Neuroreport. 9(12). 2803–2807. 95 indexed citations

Lockwood, Alan H., et al.. (1998). The functional neuroanatomy of tinnitus. Neurology. 50(1). 114–120. 476 indexed citations

Cohn, H. N., P. M. Lugger, B. W. Murphy, et al.. (1997). The Dynamics of M15: Observations of the Velocity Dispersion Profile and Fokker‐Planck Models. The Astrophysical Journal. 481(1). 267–281. 43 indexed citations

Klis, M. van der, G. Hasinger, Tadayasu Dotani, et al.. (1993). Simultaneous ROSAT/Ginga observations of 4U 1820 - 30. Monthly Notices of the Royal Astronomical Society. 260(3). 686–692. 18 indexed citations

10.

Murphy, B. W., et al.. (1993). Signal-to-noise measures for magnetic resonance imagers. Magnetic Resonance Imaging. 11(3). 425–428. 67 indexed citations

11.

Lockwood, Alan H., et al.. (1993). Positron-emission tomographic localization of abnormalities of brain metabolism in patients with minimal hepatic encephalopathy. Hepatology. 18(5). 1061–1068. 83 indexed citations

12.

Durisen, R. H., et al.. (1992). Ballistic transport in planetary ring systems due to particle erosion mechanisms. Icarus. 100(2). 364–393. 54 indexed citations

13.

Cohn, H. N., et al.. (1992). Evolving, dynamical models for collapsed-core globular clusters - M15 and NGC 6624. The Astrophysical Journal. 392. 86–86. 23 indexed citations

14.

Murphy, B. W., H. N. Cohn, & R. H. Durisen. (1991). Dynamical and luminosity evolution of active galactic nuclei - Models with a mass spectrum. The Astrophysical Journal. 370. 60–60. 81 indexed citations

15.

Hut, Piet, B. W. Murphy, & F. Verbunt. (1991). The formation rate of low-mass X-ray binaries in globular clusters. 241(1). 137–141. 2 indexed citations

16.

Murphy, B. W., R. G. M. Rutten, P. J. Callanan, et al.. (1991). Detection of binaries in the core of the globular cluster M15 using calcium emission lines. Nature. 351(6322). 130–132. 4 indexed citations

17.

Murphy, B. W., H. N. Cohn, & Piet Hut. (1990). Realistic models for evolving globular clusters. II, Post core collapse with a mass spectrum. Monthly Notices of the Royal Astronomical Society. 245(2). 335–349. 25 indexed citations

18.

Hutchins, Gary D., W.L. Rogers, Ping-Chun Chiao, Raymond R. Raylman, & B. W. Murphy. (1990). Constrained least squares filtering in high resolution PET and SPECT imaging. IEEE Transactions on Nuclear Science. 37(2). 647–651. 3 indexed citations

19.

Durisen, R. H., et al.. (1989). Ballistic transport in planetary ring systems due to particle erosion mechanisms. Icarus. 80(1). 136–166. 45 indexed citations

20.

Hearshen, David, Paul L. Carson, Paul Shreve, et al.. (1986). Automated analysis of multiple performance characteristics in magnetic resonance imaging systems. Medical Physics. 13(6). 815–823. 13 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.

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