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: Mancuso, Giulio Cesare, Altamirano, Diego, García, Federico, Lyu, Ming, Méndez, Mariano R., Combi, Jorge Ariel, Díaz Trigo, M., Zand, Jean J. M. in't
Formato: Articulo
Lenguaje:Inglés
Publicado: 2019
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125605
Aporte de:
id I19-R120-10915-125605
record_format dspace
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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