Modeling the Upper kHz QPOs of 4U 1728-34 with X-Ray Reverberation
- DOI
- 10.3847/1538-4357/ab6597
- Published
- 2020-02-01
- Container
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.3847/1538-4357/ab6597,
title = {Modeling the Upper kHz QPOs of 4U 1728-34 with X-Ray Reverberation},
author = {Benjamin M. Coughenour and Edward M. Cackett and Philippe Peille and Jon S. Troyer},
year = {2020},
journal = {The Astrophysical Journal},
doi = {10.3847/1538-4357/ab6597},
url = {https://doi.org/10.3847/1538-4357/ab6597}
}RIS
TY - JOUR TI - Modeling the Upper kHz QPOs of 4U 1728-34 with X-Ray Reverberation AU - Benjamin M. Coughenour AU - Edward M. Cackett AU - Philippe Peille AU - Jon S. Troyer PY - 2020 JO - The Astrophysical Journal DO - 10.3847/1538-4357/ab6597 UR - https://doi.org/10.3847/1538-4357/ab6597 ER -
APA
Coughenour, B. M., Cackett, E. M., Peille, P., & Troyer, J. S. (2020). Modeling the Upper kHz QPOs of 4U 1728-34 with X-Ray Reverberation. The Astrophysical Journal. https://doi.org/10.3847/1538-4357/ab6597
Source records
- crossref · retrieved 2026-11-10T11:47:45.355Z