Countries citing papers authored by B. E. Westerlund
Since
Specialization
Citations
This map shows the geographic impact of B. E. Westerlund'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. E. Westerlund with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. E. Westerlund more than expected).
Fields of papers citing papers by B. E. Westerlund
This network shows the impact of papers produced by B. E. Westerlund. 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. E. Westerlund. The network helps show where B. E. Westerlund may publish in the future.
Co-authorship network of co-authors of B. E. Westerlund
This figure shows the co-authorship network connecting the top 25 collaborators of B. E. Westerlund.
A scholar is included among the top collaborators of B. E. Westerlund 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. E. Westerlund. B. E. Westerlund is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Plez, B., et al.. (1994). On the spectra and photometry of M-giant stars. Astronomy & Astrophysics Supplement Series. 105(2). 311–336.8 indexed citations
4.
Azzopardi, M., et al.. (1993). Carbon stars in the Small Magellanic Cloud. II: Catalogue of 1707 objects with identifications and spectrophotometry. Astronomy & Astrophysics Supplement Series. 97(3). 603–728.
Winter, D. de, et al.. (1990). The extinction law, the distance and the HR diagram of the extremely young open cluster NGC 6611. Astronomy & Astrophysics Supplement Series. 82(2). 319–330.2 indexed citations
7.
Westerlund, B. E., et al.. (1990). The Evolution of Carbon Stars in the Magellanic Clouds. Astronomy & Astrophysics Supplement Series. 91(3). 338–451.1 indexed citations
8.
Deharveng, L., J. Caplan, J. Lequeux, et al.. (1988). H II regions in NGC 300.. Astronomy & Astrophysics Supplement Series. 73(3). 407–423.1 indexed citations
9.
Westerlund, B. E.. (1987). Photometry and spectroscopy of stars in the region of a highly reddened cluster in Ara.. Astronomy & Astrophysics Supplement Series. 70(3). 311–324.2 indexed citations
10.
Westerlund, B. E., et al.. (1983). Discovery of a Wolf-Rayet star in NGC 6822.. A&A. 123. 159–161.
11.
Lauberts, A., et al.. (1979). Eight southern galaxies with strong emission-line spectra.. 35. 55.
Westerlund, B. E.. (1979). Red stars in nearby galaxies.. The Messenger. 19. 7–10.5 indexed citations
14.
Lauberts, A., et al.. (1978). Spectroscopic and photometric observations of galaxies from the ESO/Uppsala list Second catalogue. Open Repository and Bibliography (University of Liège).
15.
Fehrenbach, Ch., et al.. (1973). IAS volume 50 Cover and Front matter. Symposium - International Astronomical Union. 50. f1–f8.1 indexed citations
Westerlund, B. E., I. J. Danziger, & James Graham. (1963). Supergiant stars in the wing of the Small Magellanic Cloud. Observatory. 83. 74–79.4 indexed citations
Westerlund, B. E. & A. W. Rodgers. (1959). Wolf-Rayet stars and planetary nebulae in the Large Magellanic Cloud. Observatory. 79. 132–134.3 indexed citations
20.
Westerlund, B. E.. (1958). Relative Spectral Gradients as Measured in High-Dispersion Grating Spectra. 10. 425.
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.