Unveiling the origin of the optical and UV emission during the 2017 giant outburst of the Galactic ULX pulsar Swift J0243.6+6124 (Corrigendum)
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866913842390368256 |
|---|---|
| author | Alfonso-Garzón, J. Eijnden, J. van den Kuin, N. P. M. Fürst, F. Rouco-Escorial, A. Fabregat, J. Reig, P. Mas-Hesse, J. M. Jenke, P. A. Malacaria, C. Wilson-Hodge, C. |
| author_facet | Alfonso-Garzón, J. Eijnden, J. van den Kuin, N. P. M. Fürst, F. Rouco-Escorial, A. Fabregat, J. Reig, P. Mas-Hesse, J. M. Jenke, P. A. Malacaria, C. Wilson-Hodge, C. |
| contents | An error was detected in the code of one of the components considered to model the optical/UV emission of the Galactic ULX pulsar Swift J0243.6+6124 during its 2017 giant outburst. This led to an overestimation of the contribution from the X-ray heated surface of the Be star. The addition of the X-ray irradiation of a misaligned Be disk to our model is proposed to explain the observations. Preliminary results of the updated model provide good fit to the data. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_11316 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Unveiling the origin of the optical and UV emission during the 2017 giant outburst of the Galactic ULX pulsar Swift J0243.6+6124 (Corrigendum) Alfonso-Garzón, J. Eijnden, J. van den Kuin, N. P. M. Fürst, F. Rouco-Escorial, A. Fabregat, J. Reig, P. Mas-Hesse, J. M. Jenke, P. A. Malacaria, C. Wilson-Hodge, C. High Energy Astrophysical Phenomena An error was detected in the code of one of the components considered to model the optical/UV emission of the Galactic ULX pulsar Swift J0243.6+6124 during its 2017 giant outburst. This led to an overestimation of the contribution from the X-ray heated surface of the Be star. The addition of the X-ray irradiation of a misaligned Be disk to our model is proposed to explain the observations. Preliminary results of the updated model provide good fit to the data. |
| title | Unveiling the origin of the optical and UV emission during the 2017 giant outburst of the Galactic ULX pulsar Swift J0243.6+6124 (Corrigendum) |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2505.11316 |