GX 301-2 pre-periastron and apastron flares with MAXI
Fuente:
arXiv
Gespeichert in:
| Hauptverfasser: | , , , , , , |
|---|---|
| Format: | Preprint |
| Veröffentlicht: |
2024
|
| Schlagworte: | |
| Online-Zugang: | |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| _version_ | 1866912068922245120 |
|---|---|
| author | Torregrosa, Á. Rodes-Roca, J. J. Torrejón, J. M. Sanjurjo-Ferrín, G. Mihara, T. Nakajima, M. Sugizaki, M. |
| author_facet | Torregrosa, Á. Rodes-Roca, J. J. Torrejón, J. M. Sanjurjo-Ferrín, G. Mihara, T. Nakajima, M. Sugizaki, M. |
| contents | The bright high-mass X-ray binary GX 301-2 exhibits two periodic flare episodes along its orbit which are produced when the neutron star is close to the apastron and periastron passages. Time-resolved spectra were extracted and several models applied to describe all of them. The best description was obtained with a blackbody continuum modified by the Fe K-shell absorption edge, absorbed by a large column density on the order of $10^{23}$ cm$^{-2}$ and, if present, a Fe K$α$ fluorescent emission line. Three of the nine apastron flares were as bright as the pre-periastron flare and two of them coincided with spin-up episodes of the neutron star. This fact points to the presence of a transient disc around the neutron star as it passes through the apastron that increases the accretion process. The size of emitting region on the neutron star surface showed some variability but quite consistent with a hot spot. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_03850 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | GX 301-2 pre-periastron and apastron flares with MAXI Torregrosa, Á. Rodes-Roca, J. J. Torrejón, J. M. Sanjurjo-Ferrín, G. Mihara, T. Nakajima, M. Sugizaki, M. High Energy Astrophysical Phenomena The bright high-mass X-ray binary GX 301-2 exhibits two periodic flare episodes along its orbit which are produced when the neutron star is close to the apastron and periastron passages. Time-resolved spectra were extracted and several models applied to describe all of them. The best description was obtained with a blackbody continuum modified by the Fe K-shell absorption edge, absorbed by a large column density on the order of $10^{23}$ cm$^{-2}$ and, if present, a Fe K$α$ fluorescent emission line. Three of the nine apastron flares were as bright as the pre-periastron flare and two of them coincided with spin-up episodes of the neutron star. This fact points to the presence of a transient disc around the neutron star as it passes through the apastron that increases the accretion process. The size of emitting region on the neutron star surface showed some variability but quite consistent with a hot spot. |
| title | GX 301-2 pre-periastron and apastron flares with MAXI |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2410.03850 |