Frank N. Bash

1.4k total citations
46 papers, 852 citations indexed

About

Frank N. Bash is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, Frank N. Bash has authored 46 papers receiving a total of 852 indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 13 papers in Instrumentation and 10 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in Frank N. Bash's work include Astrophysics and Star Formation Studies (16 papers), Stellar, planetary, and galactic studies (15 papers) and Astronomy and Astrophysical Research (13 papers). Frank N. Bash is often cited by papers focused on Astrophysics and Star Formation Studies (16 papers), Stellar, planetary, and galactic studies (15 papers) and Astronomy and Astrophysical Research (13 papers). Frank N. Bash collaborates with scholars based in United States, China and Australia. Frank N. Bash's co-authors include J. N. Douglas, Geoffrey W. Torrence, F. A. Bozyan, T. G. Barnes, David Leisawitz, P. Thaddeus, Michele Kaufman, F. P. Israel, W. F. Wall and D. T. Jaffe and has published in prestigious journals such as Nature, The Astrophysical Journal and Physics Today.

In The Last Decade

Frank N. Bash

40 papers receiving 823 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
Frank N. Bash United States	14	809	267	130	57	53	46	852
M. J. Reid United States	13	900 1.1×	175 0.7×	152 1.2×	31 0.5×	64 1.2×	20	919
K. Serkowski United States	15	1.0k 1.3×	192 0.7×	177 1.4×	45 0.8×	38 0.7×	56	1.1k
K. Y. Lo United States	20	1.3k 1.7×	265 1.0×	201 1.5×	80 1.4×	151 2.8×	68	1.4k
D. van Buren United States	15	778 1.0×	119 0.4×	87 0.7×	53 0.9×	57 1.1×	45	834
S. N. Tandon India	14	496 0.6×	160 0.6×	161 1.2×	45 0.8×	20 0.4×	54	604
M. Różyczka Poland	19	1.2k 1.5×	298 1.1×	117 0.9×	19 0.3×	71 1.3×	73	1.3k
C. R. Purton Canada	14	1.0k 1.3×	319 1.2×	162 1.2×	18 0.3×	44 0.8×	42	1.1k
L. M. Newton Australia	12	628 0.8×	84 0.3×	103 0.8×	67 1.2×	57 1.1×	28	658
E. B. Fomalont United States	17	739 0.9×	365 1.4×	101 0.8×	26 0.5×	32 0.6×	50	766
L. Carrasco Mexico	23	1.3k 1.6×	223 0.8×	348 2.7×	51 0.9×	36 0.7×	88	1.3k

Countries citing papers authored by Frank N. Bash

Since Specialization

Citations

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

Fields of papers citing papers by Frank N. Bash

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Frank N. Bash. 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 Frank N. Bash. The network helps show where Frank N. Bash may publish in the future.

Co-authorship network of co-authors of Frank N. Bash

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

All Works

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20 of 20 papers shown

Bash, Frank N., Karl Gebhardt, W. M. Goss, & Paul A. Vanden Bout. (2007). VERY LARGE ARRAY LIMITS FOR INTERMEDIATE-MASS BLACK HOLES IN THREE GLOBULAR CLUSTERS. The Astronomical Journal. 135(1). 182–186. 20 indexed citations

Barnes, T. G. & Frank N. Bash. (2005). Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in honor of David L. Lambert. ASPC. 336. 89 indexed citations

Booth, John A., Marsha J. Wolf, James R. Fowler, et al.. (2003). The Hobby-Eberly Telescope Completion Project. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4837. 919–919. 10 indexed citations

Sebring, Thomas A., Gil Moretto, Frank N. Bash, Frank B. Ray, & L. W. Ramsey. (2000). The Extremely Large Telescope (ELT), a scientific opportunity; an engineering certainty. European Southern Observatory Conference and Workshop Proceedings. 57. 53. 4 indexed citations

Bash, Frank N., Thomas A. Sebring, Frank B. Ray, & Lawrence W. Ramsey. (1997). <title>Extremely large telescope: a twenty-five meter aperture for the twenty-first century</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 2871. 576–584. 6 indexed citations

Bash, Frank N., R. Buta, & H. G. Corwin. (1996). Gérard H. de Vaucouleurs. Physics Today. 49(4). 76–76. 1 indexed citations

Walker, Constance E., et al.. (1992). The Starburst Properties of M82, M83, and IC342. American Astronomical Society Meeting Abstracts. 181. 203–206. 2 indexed citations

Li, Zongwei, J. C. Wheeler, Frank N. Bash, & W. H. Jefferys. (1988). A Statistical Study of the Correlation of Galactic Supernova Remnants and Spiral Arms. International Astronomical Union Colloquium. 101. 485–488. 1 indexed citations

Kaufman, Michele, Frank N. Bash, Jr. Kennicutt R. C., & P. W. Hodge. (1987). Giant H II regions in M81. The Astrophysical Journal. 319. 61–61. 31 indexed citations

10.

Peters, W. L. & Frank N. Bash. (1987). The correlation of spiral arm molecular clouds with cold atomic hydrogen. The Astrophysical Journal. 317. 646–646. 7 indexed citations

11.

Bash, Frank N. & Michele Kaufman. (1986). The global spiral structure of M81 - Radio continuum maps. The Astrophysical Journal. 310. 621–621. 14 indexed citations

12.

Bash, Frank N.. (1986). The present, past and future velocity of nearby stars: the path of the Sun in 10 8 years.. 35–46. 1 indexed citations

13.

Peters, W. L. & Frank N. Bash. (1983). CO Emission vs HI Self-Absorption. Publications of the Astronomical Society of Australia. 5(2). 224–227. 1 indexed citations

14.

Leisawitz, David & Frank N. Bash. (1982). Implications of collisionally supported giant molecular clouds for spiral galactic structure and massive star formation. The Astrophysical Journal. 259. 133–133. 2 indexed citations

15.

Douglas, J. N., et al.. (1980). The Texas Survey: Preliminary +18°\ Strip. 17. 1. 1 indexed citations

16.

Wills, Beverley J., Alan Uomoto, Steven S. Vogt, et al.. (1977). An Observational Model of the Ionized Gas in Seyfert and Radio-Galaxy Nuclei. Bulletin of the American Astronomical Society. 9. 647. 1 indexed citations

17.

Bash, Frank N., et al.. (1977). The galactic density wave, molecular clouds, and star formation. The Astrophysical Journal. 217. 464–464. 33 indexed citations

18.

Bash, Frank N., et al.. (1976). Dynamics of CO molecular clouds in the galaxy. The Astrophysical Journal. 205. 786–786. 11 indexed citations

19.

Bash, Frank N., et al.. (1975). Positions and flux densities of 1075 radio sources at 365 MHz. The Astronomical Journal. 80. 335–335. 1 indexed citations

20.

Bash, Frank N. & F. D. Ghigo. (1973). Recent Observations of Cyg X-3 at 365 MHz. Nature Physical Science. 241(109). 93–94. 3 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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