W. J. Henney
About
In The Last Decade
W. J. Henney
62 papers receiving 1.5k citations
Hit Papers
Peers
Comparison fields: 5 of 30
- Astronomy and Astrophysics 1.5k
- Spectroscopy 186
- Instrumentation 144
- Nuclear and High Energy Physics 110
- Atomic and Molecular Physics, and Optics 99
Countries citing papers authored by W. J. Henney
This map shows the geographic impact of W. J. Henney'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 W. J. Henney with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. J. Henney more than expected).
Fields of papers citing papers by W. J. Henney
This network shows the impact of papers produced by W. J. Henney. 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 W. J. Henney. The network helps show where W. J. Henney may publish in the future.
Co-authorship network of co-authors of W. J. Henney
This figure shows the co-authorship network connecting the top 25 collaborators of W. J. Henney. A scholar is included among the top collaborators of W. J. Henney 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 W. J. Henney. W. J. Henney is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 18 | |
| 3 | 8 | |
| 4 | The abundance discrepancy factor and t^2 in nebulae: are non-thermal electrons the culprits? | 10 |
| 5 | Studies of NGC 6720 with Calibrated <em>HST</em>/WFC3 Emission-line Filter Images. I. Structure and Evolution | 16 |
| 6 | Studies of NGC 6720 with Calibrated <em>HST</em>/WFC3 Emission-line Filter Images. II. Physical Conditions | 6 |
| 7 | The 2013 Release of Cloudy breakdown → | 410 |
| 8 | 92 | |
| 9 | 14 | |
| 10 | Winds, bubbles, and explosions : a conference to honor John Dyson | 2 |
| 11 | Determination of the Electron Density in the Orion Nebula with High Spectral Resolution | 2 |
| 12 | LARGE-SCALE PHOTOEVAPORATION FLOWS IN H II REGIONS | 2 |
| 13 | Knots in Planetary Nebulae | 2 |
| 14 | Emission lines from jet flows | 10 |
| 15 | Mass Loading by Proplyds of an O-Star Wind | 2 |
| 16 | Multiple flow interactions in a proplyd binary system I. The interproplyd shell | 4 |
| 17 | An ionized microjet from the orion nebula proplyd LV 2 | 1 |
| 18 | Ionized photoevaporation flows in h II regions and PNe | 2 |
| 19 | 104 | |
| 20 | Emission line images and spectra of asymmetric bowshocks | 1 |
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.