{ "id": "2105.12338", "version": "v1", "published": "2021-05-26T05:38:36.000Z", "updated": "2021-05-26T05:38:36.000Z", "title": "NICER uncovers the transient nature of the type-B quasi-periodic oscillation in the black hole candidate MAXI J1348-630", "authors": [ "L. Zhang", "D. Altamirano", "P. Uttley", "F. Garcia", "M. Mendez", "J. Homan", "J. F. Steiner", "K. Alabarta", "D. J. K. Buisson", "R. A. Remillard", "K. C. Gendreau", "Z. Arzoumanian", "C. Markwardt", "T. E. Strohmayer", "J. Neilsen", "A. Basak" ], "comment": "23 pages, 12 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We present a systematic spectral-timing analysis of a fast appearance/disappearance of a type-B quasi-periodic oscillation (QPO), observed in four NICER observations of MAXI J1348-630. By comparing the spectra of the period with and without the type-B QPO, we found that the main difference appears at energy bands above ~2 keV, suggesting that the QPO emission is dominated by the hard Comptonised component. During the transition, a change in the relative contribution of the disk and Comptonised emission was observed. The disk flux decreased while the Comptonised flux increased from non-QPO to type-B QPO. However, the total flux did not change too much in the NICER band. Our results reveal that the type-B QPO is associated with a redistribution of accretion power between the disk and Comptonised emission. When the type-B QPO appears, more accretion power is dissipated into the Comptonised region than in the disk. Our spectral fits give a hint that the increased Comptonised emission may come from an additional component that is related to the base of the jet.", "revisions": [ { "version": "v1", "updated": "2021-05-26T05:38:36.000Z" } ], "analyses": { "keywords": [ "black hole candidate maxi", "type-b quasi-periodic oscillation", "transient nature", "type-b qpo", "nicer uncovers" ], "note": { "typesetting": "TeX", "pages": 23, "language": "en", "license": "arXiv", "status": "editable" } } }