Published September 3, 2022
| Version v1
Poster
Open
The mass of the white dwarf in GK Per
Creators
- 1. Instituto de Astrofísica de Canarias / Departamento de Astrofísica, Universidad de La Laguna
- 2. Indian institute of astrophysics
- 3. Section of Astrophysics, Astronomy and Mechanics, Department of Physics, National and Kapodistrian University of Athens
- 4. Indian institute of astrophysics / Department of Physics, Pondicherry University
- 5. Dept. of Physics & Astrophysics, University Road, University Enclave
- 6. Finnish Centre for Astronomy with ESO (FINCA), Quantum, University of Turku
- 7. First Light Observatory Systems
- 8. Center for Astrophysics | Harvard & Smithsonian
- 9. SRON, Netherlands Institute for Space Research / Department of Astrophysics, IMAPP, Radboud University
- 10. CAS Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences
- 11. Anton Pannekoek Institute, University of Amsterdam / ASTRON, the Netherlands Institute for Radio Astronomy
- 12. American Association of Variable Star Observers
- 13. European Southern Observatory
Description
Poster contribution to the XV Scientific Meeting of the Sociedad Española de Astronomía (2022). We present a dynamical study of the cataclysmic variable GK Per, comparing our dynamical white dwarf mass with several estimates obtained from indirect methods.
Files
Poster-SEA2022-GKPer.pdf
Files
(1.2 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:af9ca1cf6e4baa55d7e767e73a8b5238
|
1.2 MB | Preview Download |