C. Henkel

Max Planck Institute for Radio Astronomy

Papers

1

Total Citations

2

H-Index

1

About

C. Henkel is an observational astronomer whose research centers on the structure and evolution of galaxies, with a particular focus on the faint tidal features that reveal their merger histories. Henkel’s major contribution lies in demonstrating that deep imaging from small, amateur-class telescopes can rival professional observatories in detecting stellar streams and diffuse structures around nearby galaxies. This breakthrough has opened a new, accessible frontier for studying galaxy interactions and the hierarchical assembly predicted by ΛCDM cosmology. In their most-cited work (2025, 2 citations), Henkel and collaborators used a network of amateur instruments to map tidal streams around spiral galaxies beyond the Local Group, showing that these delicate features preserve the fossil record of past satellite accretions. Though early in their career, Henkel’s approach has already influenced how the community leverages citizen science and low-cost equipment for high-impact extragalactic research. Their work bridges professional astronomy and public engagement, making the study of galaxy evolution more democratic and data-rich.

Research Focus

Key Achievements

1
H-Index
1
Papers
2
Total Citations
2
Avg Citations/Paper
🏆 Most Cited Paper
Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes
2 citations · 2025
📈 Most Prolific Year: 2025 (1 Papers)
🤝 Key Collaborators: 27
🏛 Institutions: Max Planck Institute for Radio Astronomy

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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