The nature of the X-ray binary transient MAXI J1834-021: Clues from its first observed outburst
MAXI J1834- 021 is a new X-ray transient discovered in February 2023. We analysed the spectral and timing properties of MAXI J1834- 021 using NICER, NuSTAR and Swift data collected between March and October 2023. The light curve showed a main peak followed by a second activity phase. Most of the spe...
| Autores: | , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/400391 |
| Acceso en línea: | http://hdl.handle.net/10261/400391 https://api.elsevier.com/content/abstract/scopus_id/105010090901 |
| Access Level: | acceso abierto |
| Palabra clave: | Accretion, accretion disks Binaries: general Stars: black holes Stars: low-mass X-rays: individuals: MAXI J1834- 021 |
| Sumario: | MAXI J1834- 021 is a new X-ray transient discovered in February 2023. We analysed the spectral and timing properties of MAXI J1834- 021 using NICER, NuSTAR and Swift data collected between March and October 2023. The light curve showed a main peak followed by a second activity phase. Most of the spectra extracted from individual NICER observations could be adequately fit with a Comptonisation component alone, while some required an additional thermal component. The spectral evolution is consistent with a softening trend as the source becomes brighter in X-rays. We also analysed the broadband spectrum by combining data from simultaneous NICER and NuSTAR observations on March 10, 2023. This spectrum can be fitted with a disc component having an inner radius temperature of kT<inf>in</inf>∼0.4 keV and a Comptonisation component with a power-law photon index of Γ ∼1.8. By including a reflection component in the modelling, we obtained a 3σ upper limit for the inner disc radius of 11.4 gravitational radii. We also detected a quasi-periodic oscillation (QPO), whose central frequency varies with time (from 2 Hz to ∼0.9 Hz), and anti-correlates with the hardness ratio. Based on the observed spectral-timing properties, MAXI J1834- 021 can be classified as a low-mass X-ray binary in outburst. However, we cannot draw a definitive conclusion about the nature of the accreting compact object, which could currently be a black hole or a neutron star. |
|---|