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http://hdl.handle.net/2289/8163
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DC Field | Value | Language |
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dc.contributor.author | Sharma, Rahul | - |
dc.contributor.author | Jain, Chetana | - |
dc.contributor.author | Paul, Biswajit | - |
dc.contributor.author | Seshadri, T. R. | - |
dc.date.accessioned | 2023-10-27T06:31:32Z | - |
dc.date.available | 2023-10-27T06:31:32Z | - |
dc.date.issued | 2023-10-01 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2023, Vol. 526, p4877 | en_US |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.issn | 1365-2966 (Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/8163 | - |
dc.description | Open Access | en_US |
dc.description.abstract | We present here timing and spectral analyses of SGR J1830−0645 based on an AstroSat observation carried out on 2020 October 16, about a week after the onset of its first detected X-ray outburst. Using data taken with the Soft X-ray Telescope (SXT) and Large Area X-ray Proportional Counter (LAXPC), we have detected 0.9–10 keV coherent pulsations at a period of ∼10.4 s. The pulse profiles were single-peaked, asymmetric, and consisted of minor peaks attributable to hotspots on the neutron star surface. The pulsed fraction evolved significantly with energy, increasing to energies around 5 keV with a steep drop thereafter. The 0.9–25 keV SXT–LAXPC energy spectrum is best described with two thermal components having temperatures ∼0.46 and ∼1.1 keV (emission radii of ∼2.4 and ∼0.65 km, respectively, assuming a distance of 4 kpc) along with a power-law component having a photon index of ∼0.39. We report the detection of 67 X-ray bursts having an average duration of ∼33 ms. The brightest burst lasted for about 90 ms and had a 3–25 keV fluence of ∼5 × 10−9 erg cm−2 . | en_US |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press on behalf of Royal Astronomical Society | en_US |
dc.relation.uri | https://ui.adsabs.harvard.edu/abs/2023arXiv231004079S/abstract | en_US |
dc.relation.uri | https://arxiv.org/abs/2310.04079 | en_US |
dc.relation.uri | https://doi.org/10.1093/mnras/stad3026 | en_US |
dc.relation.uri | https://inspirehep.net/literature/2709449 | en_US |
dc.rights | 2023 The Author(s) | en_US |
dc.subject | stars | en_US |
dc.subject | neutron | en_US |
dc.subject | magnetars | en_US |
dc.subject | x-rays | en_US |
dc.subject | bursts | en_US |
dc.subject | SGR J1830−0645 | en_US |
dc.title | AstroSat observation of the magnetar SGR J1830−0645 during its first detected X-ray outburst | en_US |
dc.type | Article | en_US |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2023_MNRAS_Vol.526_p4877.pdf Restricted Access | Open Access | 1.28 MB | Adobe PDF | View/Open Request a copy |
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