Gravitational torques from lopsided young stellar component sustain high black hole accretion rates in NGC 4593
- DOI
- 10.1051/0004-6361/202553991
- Published
- 2025-08
- Container
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.1051/0004-6361/202553991,
title = {Gravitational torques from lopsided young stellar component sustain high black hole accretion rates in NGC 4593},
author = {N. Winkel and K. Jahnke and J. A. Fernández-Ontiveros and T. A. Davis and F. Combes and M. Gaspari and J. Neumann and M. Singha and J. S. Elford and V. N. Bennert and M. A. Malkan},
year = {2025},
journal = {Astronomy \& Astrophysics},
doi = {10.1051/0004-6361/202553991},
url = {https://doi.org/10.1051/0004-6361/202553991}
}RIS
TY - JOUR TI - Gravitational torques from lopsided young stellar component sustain high black hole accretion rates in NGC 4593 AU - N. Winkel AU - K. Jahnke AU - J. A. Fernández-Ontiveros AU - T. A. Davis AU - F. Combes AU - M. Gaspari AU - J. Neumann AU - M. Singha AU - J. S. Elford AU - V. N. Bennert AU - M. A. Malkan PY - 2025 JO - Astronomy & Astrophysics DO - 10.1051/0004-6361/202553991 UR - https://doi.org/10.1051/0004-6361/202553991 ER -
APA
Winkel, N., Jahnke, K., Fernández-Ontiveros, J. A., Davis, T. A., Combes, F., Gaspari, M., Neumann, J., Singha, M., Elford, J. S., Bennert, V. N., & Malkan, M. A. (2025). Gravitational torques from lopsided young stellar component sustain high black hole accretion rates in NGC 4593. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/202553991
Source records
- crossref · retrieved 2026-09-27T05:05:01.352Z