Published February 14, 2024
| Version v2
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Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
Authors/Creators
- 1. Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, the Netherlands
- 2. Independent researcher
- 3. School of Physics & Astronomy, Monash University, Clayton, VIC 3800, Australia
- 4. ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL, Nijmegen, The Netherlands
- 5. Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA
- 6. Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85741 Garching, Germany
- 7. University of Tuebingen: Tuebingen, DE
Description
Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
Files
Mass_radius_contours.zip
Additional details
Dates
- Accepted
-
2025-02-11