C. Buchbender

1.8k total citations
27 papers, 291 citations indexed

About

C. Buchbender is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, C. Buchbender has authored 27 papers receiving a total of 291 indexed citations (citations by other indexed papers that have themselves been cited), including 26 papers in Astronomy and Astrophysics, 7 papers in Spectroscopy and 6 papers in Atmospheric Science. Recurrent topics in C. Buchbender's work include Astrophysics and Star Formation Studies (24 papers), Stellar, planetary, and galactic studies (15 papers) and Galaxies: Formation, Evolution, Phenomena (9 papers). C. Buchbender is often cited by papers focused on Astrophysics and Star Formation Studies (24 papers), Stellar, planetary, and galactic studies (15 papers) and Galaxies: Formation, Evolution, Phenomena (9 papers). C. Buchbender collaborates with scholars based in Germany, United States and France. C. Buchbender's co-authors include J. Stützki, R. Güsten, N. Schneider, A. G. G. M. Tielens, R. Higgins, R. Simon, C. Krämer, M. Röllig, H. Wiesemeyer and Heiko Richter and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

C. Buchbender

22 papers receiving 256 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
C. Buchbender Germany 12 258 74 47 32 15 27 291
H. Jakob Germany 6 183 0.7× 58 0.8× 31 0.7× 26 0.8× 12 0.8× 15 210
Pieter Deroo United States 5 171 0.7× 75 1.0× 78 1.7× 38 1.2× 8 0.5× 14 231
R. Higgins Germany 9 210 0.8× 130 1.8× 82 1.7× 53 1.7× 8 0.5× 29 301
Hiroshige Yoshida United States 6 246 1.0× 53 0.7× 51 1.1× 28 0.9× 16 1.1× 16 263
Maohai Huang China 8 171 0.7× 72 1.0× 49 1.0× 21 0.7× 9 0.6× 19 199
J.‐P. Baluteau France 8 114 0.4× 53 0.7× 45 1.0× 23 0.7× 14 0.9× 15 138
A. M. Di Giorgio Italy 8 326 1.3× 90 1.2× 49 1.0× 16 0.5× 11 0.7× 33 346
Masuo Tanaka Japan 12 310 1.2× 94 1.3× 74 1.6× 49 1.5× 11 0.7× 35 349
Polychronis Patapis Switzerland 7 146 0.6× 31 0.4× 26 0.6× 25 0.8× 14 0.9× 17 177
R. Vavrek Netherlands 11 335 1.3× 74 1.0× 39 0.8× 14 0.4× 5 0.3× 27 354

Countries citing papers authored by C. Buchbender

Since Specialization
Citations

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

Fields of papers citing papers by C. Buchbender

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. Buchbender. 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 C. Buchbender. The network helps show where C. Buchbender may publish in the future.

Co-authorship network of co-authors of C. Buchbender

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

All Works

20 of 20 papers shown
1.
Okada, Yoko, R. Güsten, V. Ossenkopf, et al.. (2024). Bright-rimmed clouds in IC 1396. Astronomy and Astrophysics. 690. A45–A45.
2.
Buchbender, C., V. Ossenkopf, N. Schneider, et al.. (2024). Molecular cloud matching in CO and dust in M33. Astronomy and Astrophysics. 688. A171–A171. 2 indexed citations
3.
Schneider, N., S. Bontemps, R. Simon, et al.. (2023). Ionized carbon as a tracer of the assembly of interstellar clouds. Nature Astronomy. 7(5). 546–556. 16 indexed citations
4.
Schneider, N., A. Zavagno, R. Simon, et al.. (2023). The SOFIA FEEDBACK [CII] Legacy Survey: Rapid molecular cloud dispersal in RCW 79. Astronomy and Astrophysics. 679. L5–L5. 5 indexed citations
5.
Beuther, H., N. Schneider, R. Simon, et al.. (2022). FEEDBACK from the NGC 7538 H II region. Astronomy and Astrophysics. 659. A77–A77. 18 indexed citations
6.
Wolfire, M. G., Marc W. Pound, C. Buchbender, et al.. (2022). SOFIA FEEDBACK Survey: PDR Diagnostics of Stellar Feedback in Different Regions of RCW 49. The Astronomical Journal. 164(4). 150–150. 5 indexed citations
7.
Langer, W. D., J. L. Pineda, P. F. Goldsmith, et al.. (2021). The dense warm ionized medium in the inner Galaxy. Astronomy and Astrophysics. 651. A59–A59. 6 indexed citations
8.
Higgins, R., D. Teyssier, J. R. Goicoechea, et al.. (2021). Observation and calibration strategies for large-scale multi-beam velocity-resolved mapping of the [CII] emission in the Orion molecular cloud. Springer Link (Chiba Institute of Technology). 6 indexed citations
9.
Pound, Marc W., M. G. Wolfire, C. Buchbender, et al.. (2021). SOFIA FEEDBACK Survey: Exploring the Dynamics of the Stellar Wind–Driven Shell of RCW 49. The Astrophysical Journal. 914(2). 117–117. 25 indexed citations
10.
Anderson, L. D., N. Schneider, R. Simon, et al.. (2021). Stellar feedback and triggered star formation in the prototypical bubble RCW 120. HAL (Le Centre pour la Communication Scientifique Directe). 33 indexed citations
11.
Kirsanova, M. S., V. Ossenkopf, L. D. Anderson, et al.. (2020). The PDR structure and kinematics around the compact H ii regions S235 A and S235 C with [C ii], [13C ii], [O i], and HCO+ line profiles. Monthly Notices of the Royal Astronomical Society. 497(3). 2651–2669. 18 indexed citations
12.
Goicoechea, J. R., N. Marcelino, A. G. G. M. Tielens, et al.. (2020). Molecular globules in the Veil bubble of Orion. Astronomy and Astrophysics. 639. A1–A1. 18 indexed citations
13.
Krämer, C., Thomas Nikola, S. Anderl, et al.. (2020). Gas and dust cooling along the major axis of M 33 (HerM33es). Astronomy and Astrophysics. 639. A61–A61. 9 indexed citations
14.
Simon, R., N. Schneider, Frank Bigiel, et al.. (2019). The Cycling of Matter from the Interstellar Medium to Stars and back. Bulletin of the American Astronomical Society. 51(3). 367. 1 indexed citations
15.
Schneider, N., M. Röllig, E. T. Polehampton, et al.. (2017). Globules and pillars in Cygnus X. Springer Link (Chiba Institute of Technology). 7 indexed citations
16.
Relaño, M., S. Verley, Isabel Pérez, et al.. (2013). Spectral energy distributions of H ii regions in M 33 (HerM33es). Astronomy and Astrophysics. 552. A140–A140. 13 indexed citations
17.
Krämer, C., S. García‐Burillo, M. Relaño, et al.. (2013). Gas and dust cooling along the major axis of M 33 (HerM33es). Astronomy and Astrophysics. 553. A114–A114. 11 indexed citations
18.
Buchbender, C., C. Krämer, M. C. González-García, et al.. (2012). Dense gas in M 33 (HerM33es). Astronomy and Astrophysics. 549. A17–A17. 17 indexed citations
19.
Boquien, M., Daniela Calzetti, C. Krämer, et al.. (2010). 100 μm and 160 μm emission as resolved star-formation rate estimators in M 33 (HERM33ES). Astronomy and Astrophysics. 518. L70–L70. 14 indexed citations
20.
Verley, S., M. Relaño, C. Krämer, et al.. (2010). Properties of compact 250μm emission and H II regions in M 33 (HERM33ES). Astronomy and Astrophysics. 518. L68–L68. 11 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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2026