{ "id": "2304.06077", "version": "v1", "published": "2023-04-12T18:00:05.000Z", "updated": "2023-04-12T18:00:05.000Z", "title": "A journey from the hard to the soft state: How do QPOs evolve in the 2021 outburst of GX 339-4?", "authors": [ "H. Stiele", "A. K. H. Kong" ], "comment": "6 pages, 5 figures, supplementary online material as appendices (13 pages), accepted for publication in MNRAS", "doi": "10.1093/mnras/stad969", "categories": [ "astro-ph.HE" ], "abstract": "We investigated the snapshots of five NICER observations of the black hole transient GX 339-4 when the source transited from the hard state into the soft state during its outburst in 2021. In this paper, we focused our study on the evolution of quasi-periodic oscillations (QPOs) and noise components using power-density spectra. In addition, we derived hardness ratios comparing count rates above and below 2 keV. The evolution from the hard to the soft state was a somewhat erratic process showing several transitions between states that are dominated by top-flat noise and can show type-C QPOs; those that are dominated by red noise and can show type-B QPOs. From the parameters that we studied, we only found a strong correlation between the hardness ratio and the type of QPO observed. This implies that the appearance of type-B QPOs is related to a change in the accretion geometry of the system that also reflects in altered spectral properties. We also observed that the type-B QPO forms from or disintegrates into a broad peaked feature when the source comes out of or goes to the hard-intermediate state, respectively. This implies some strong decoherence in the process that creates this feature.", "revisions": [ { "version": "v1", "updated": "2023-04-12T18:00:05.000Z" } ], "analyses": { "keywords": [ "soft state", "qpos evolve", "black hole transient gx", "type-b qpo forms", "somewhat erratic process" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }