This map shows the geographic impact of B. Stenholm'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. Stenholm with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Stenholm more than expected).
This network shows the impact of papers produced by B. Stenholm. 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. Stenholm. The network helps show where B. Stenholm may publish in the future.
Co-authorship network of co-authors of B. Stenholm
This figure shows the co-authorship network connecting the top 25 collaborators of B. Stenholm.
A scholar is included among the top collaborators of B. Stenholm 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. Stenholm. B. Stenholm is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Schrijver, H., et al.. (1998). Wolf-Rayet stars and O-star runaways with HIPPARCOS - II. Photometry. University of Groningen research database (University of Groningen / Centre for Information Technology). 331(3). 1022–1036.2 indexed citations
Tylenda, R., A. Acker, & B. Stenholm. (1993). Wolf-Rayet nuclei of planetary nebulae. Observations and classification.. Astronomy & Astrophysics Supplement Series. 102(3). 595–602.3 indexed citations
6.
Tylenda, R., et al.. (1992). The extinction constants for galactic planetary nebulae.. Astronomy & Astrophysics Supplement Series. 95(2). 337–354.2 indexed citations
7.
Acker, A., et al.. (1991). An extensive study of planetary nebulae in the galactic bulge. I. Spectrophotometric data.. Astronomy & Astrophysics Supplement Series. 89(2). 237–258.4 indexed citations
8.
Tylenda, R., et al.. (1991). The B and V magnitudes of the central stars of planetary nebulae.. Astronomy & Astrophysics Supplement Series. 89(1). 77–90.4 indexed citations
9.
Acker, A., et al.. (1991). The absolute H-beta fluxes for galactic planetary nebulae.. Astronomy & Astrophysics Supplement Series. 90(1). 89–101.2 indexed citations
10.
Acker, A., et al.. (1991). Spectrophotometric survey of southern planetary nebulae. II. Chemical compositions.. A&A. 248. 197.1 indexed citations
11.
Acker, A. & B. Stenholm. (1990). Misclassified planetary nebulae. Astronomy & Astrophysics Supplement Series. 86(2). 219–225.1 indexed citations
12.
Tylenda, R., et al.. (1989). Magnitudes of central stars of southern planetary nebulae. Astronomy & Astrophysics Supplement Series. 77(1). 39–44.2 indexed citations
13.
Köppen, J., et al.. (1989). On the theoretical ratio of some nebular lines.. Msngr. 58. 44–46.2 indexed citations
14.
Acker, A., et al.. (1989). The energy-balance temperature of central stars of galactic planetary nebulae.II.. Astronomy & Astrophysics Supplement Series. 81(1). 121–131.1 indexed citations
Acker, A., B. Stenholm, & R. Tylenda. (1989). The absolute H-beta fluxes for southern planetary nebulae.. Astronomy & Astrophysics Supplement Series. 77(3). 487–495.1 indexed citations
17.
Acker, A., Ingemar Lundström, & B. Stenholm. (1988). Spectrophotometry of new symbiotic stars.. Astronomy & Astrophysics Supplement Series. 73(2). 325–333.2 indexed citations
Lundström, Ingemar & B. Stenholm. (1979). Photometry and spectrography of faint Wolf-Rayet stars.. Astronomy & Astrophysics Supplement Series. 35. 303–312.
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.