Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676
We report the discovery of millihertz quasi-periodic oscillations (mHz QPOs) from the bursting, high-inclination atoll neutron star low-mass X-ray binary (NS LMXB) EXO 0748-676 with the Rossi X-ray Time Explorer (RXTE). This class of QPO, originally discovered in three NS LMXBs, has been interpreted...
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Autores principales: | , , , , , , , |
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Formato: | Articulo |
Lenguaje: | Inglés |
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2019
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125605 |
Aporte de: |
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I19-R120-10915-125605 |
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institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Astronomía accretion, accretion discs stars: individual: EXO 0748−676 stars: neutron X-rays: binaries |
spellingShingle |
Astronomía accretion, accretion discs stars: individual: EXO 0748−676 stars: neutron X-rays: binaries Mancuso, Giulio Cesare Altamirano, Diego García, Federico Lyu, Ming Méndez, Mariano R. Combi, Jorge Ariel Díaz Trigo, M. Zand, Jean J. M. in't Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
topic_facet |
Astronomía accretion, accretion discs stars: individual: EXO 0748−676 stars: neutron X-rays: binaries |
description |
We report the discovery of millihertz quasi-periodic oscillations (mHz QPOs) from the bursting, high-inclination atoll neutron star low-mass X-ray binary (NS LMXB) EXO 0748-676 with the Rossi X-ray Time Explorer (RXTE). This class of QPO, originally discovered in three NS LMXBs, has been interpreted as a consequence of a special mode of nuclear burning on the NS surface. Using all the RXTE archival observations of the source, we detected significant (>3σ) mHz QPOs in 11 observations. The frequency of the oscillations was between ∼5 and ∼13 mHz. We also found a decrease of the QPO frequency with time in two occasions; in one of these the oscillations disappeared with the onset of an X-ray burst, similar to what was reported in other sources. Our analysis of the X-ray colours revealed that EXO 0748-676 was in a soft spectral state when it exhibited the QPOs. This makes EXO 0748-676 the sixth source with mHz oscillations associated with marginally stable burning, and the second one that shows a systematic frequency drift. Our results suggest that the mechanism that produces the drift might always be present if the mHz QPOs are observed in the so-called intermediate state. |
format |
Articulo Articulo |
author |
Mancuso, Giulio Cesare Altamirano, Diego García, Federico Lyu, Ming Méndez, Mariano R. Combi, Jorge Ariel Díaz Trigo, M. Zand, Jean J. M. in't |
author_facet |
Mancuso, Giulio Cesare Altamirano, Diego García, Federico Lyu, Ming Méndez, Mariano R. Combi, Jorge Ariel Díaz Trigo, M. Zand, Jean J. M. in't |
author_sort |
Mancuso, Giulio Cesare |
title |
Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
title_short |
Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
title_full |
Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
title_fullStr |
Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
title_full_unstemmed |
Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676 |
title_sort |
discovery of millihertz quasi-periodic oscillations in the x-ray binary exo 0748−676 |
publishDate |
2019 |
url |
http://sedici.unlp.edu.ar/handle/10915/125605 |
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bdutipo_str |
Repositorios |
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1764820451934076930 |