Quenching and Recovery of Persistent X-Ray Emission during a Superburst in 4U 1820–30

Bibliographic Details
Title: Quenching and Recovery of Persistent X-Ray Emission during a Superburst in 4U 1820–30
Authors: Zhijiao Peng, Zhaosheng Li, Yuanyue Pan, Tao Fu, Wenhui Yu, Yupeng Chen, Shu Zhang, Maurizio Falanga, Shuang-Nan Zhang
Source: The Astrophysical Journal, Vol 982, Iss 1, p 18 (2025)
Publisher Information: IOP Publishing, 2025.
Publication Year: 2025
Collection: LCC:Astrophysics
Subject Terms: Low-mass x-ray binary stars, X-ray bursters, Neutron stars, Astrophysics, QB460-466
More Details: We report the superburst from 4U 1820–30 in 2021 observed by the Monitor of All-sky X-ray Image and Neutron star Interior Composition Explorer (NICER). During the tail of the superburst, we found that the NICER light curve unexpectedly increased from 1080 to 2204 counts s ^−1 over 6.89 hr. From the time-resolved superburst spectra, we estimated the burst decay time of ≈2.5 hr, the ignition column depth of ≈0.3 × 10 ^12 g cm ^−2 , the energy release per unit mass of ≈2.4 × 10 ^17 erg g ^−1 , the fluence of ≈4.1 × 10 ^−4 erg cm ^−2 , and the total energy release of ≈3.5 × 10 ^42 erg. Notably, we found a gradual increase in the Comptonization flux from 8.9 × 10 ^−10 erg s ^−1 cm ^−2 to the preburst level during the superburst. This increase can be interpreted as a consequence of superburst radiation depleting the inner accretion disk, leading to a near-complete quenching of the persistent emission. As the burst radiation decayed, the inner accretion disk gradually returned to its preburst state, as evidenced by the best-fit spectral parameters. Additionally, we observed a prominent absorption line that exhibited a gravitational redshift, shifting from 4.15 to 3.62 keV during the recovery phase of persistent emission. This absorption feature likely originates from the inner accretion disk rather than from burst emission on the neutron star (NS) surface. The observed changes in the absorption line energy suggest that the inner disk approached the NS to a distance as close as ≈17 km.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/adb726
Access URL: https://doaj.org/article/f7d560e541a44d1cb93fa35cc1e001d4
Accession Number: edsdoj.f7d560e541a44d1cb93fa35cc1e001d4
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/adb726
Published in:The Astrophysical Journal
Language:English