Saved in:
| Main Authors: | , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2402.02213 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866913227178246144 |
|---|---|
| author | Hussain, Arshad Goswami, Umananda Dev |
| author_facet | Hussain, Arshad Goswami, Umananda Dev |
| contents | A Be/X-ray binary system known as RX J0440.9+4431 (or LS V +44 17) is a potential member of the uncommon gamma-ray binary class. With an orbital period of 150 days, this system consists of a neutron star and a Be star companion. The MAXI observatory discovered an X-ray outburst from the source in December of 2022. Early in January, the outburst reached its peak, which was then followed by a decrease and a subsequent rebrightening. The X-ray flux exceeded 1 Crab in the 15-50 keV range at this second peak. AstroSat observations were conducted close to the peak of the second outburst, from January 11 to January 12, 2023. We report here the results of our search for 3-80 keV X-ray emission in the data of the AstroSat's LAXPC detector. It is found that the pulse period of the source is around 208 seconds. The source is found to be emitting more in the softer part of the X-ray energy range. The spectral characteristics can be described by employing a power-law model with an exponential cutoff, along with a blackbody component, interstellar absorption and an additional 6.4 keV iron fluorescence line. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2402_02213 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | AstroSat Observation of Recent Outburst in the Be/X-ray Binary LS V +4417/RX J0440.9+4431 Hussain, Arshad Goswami, Umananda Dev High Energy Astrophysical Phenomena A Be/X-ray binary system known as RX J0440.9+4431 (or LS V +44 17) is a potential member of the uncommon gamma-ray binary class. With an orbital period of 150 days, this system consists of a neutron star and a Be star companion. The MAXI observatory discovered an X-ray outburst from the source in December of 2022. Early in January, the outburst reached its peak, which was then followed by a decrease and a subsequent rebrightening. The X-ray flux exceeded 1 Crab in the 15-50 keV range at this second peak. AstroSat observations were conducted close to the peak of the second outburst, from January 11 to January 12, 2023. We report here the results of our search for 3-80 keV X-ray emission in the data of the AstroSat's LAXPC detector. It is found that the pulse period of the source is around 208 seconds. The source is found to be emitting more in the softer part of the X-ray energy range. The spectral characteristics can be described by employing a power-law model with an exponential cutoff, along with a blackbody component, interstellar absorption and an additional 6.4 keV iron fluorescence line. |
| title | AstroSat Observation of Recent Outburst in the Be/X-ray Binary LS V +4417/RX J0440.9+4431 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2402.02213 |