Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52

We present new Rossi X-ray Timing Explorer observations of the low-mass X-ray binary 4U 1608-52 during the decay of its 1998 outburst. We detect by a direct FFT method the existence of a second kilohertz quasi-periodic oscillation (kHz QPO) in its power density spectrum, previously only seen by mean...

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Detalles Bibliográficos
Autores principales: Méndez, Mariano R., van der Klis, Michiel, Wijnands, Rudy, Ford, Eric, van Paradijs, Jan, Vaughan, Brian A.
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 1998
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123191
Aporte de:
id I19-R120-10915-123191
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Accretion, accretion disks
Stars: neutron
Stars: individual (4 U 1608–52)
X-rays: stars
spellingShingle Ciencias Astronómicas
Accretion, accretion disks
Stars: neutron
Stars: individual (4 U 1608–52)
X-rays: stars
Méndez, Mariano R.
van der Klis, Michiel
Wijnands, Rudy
Ford, Eric
van Paradijs, Jan
Vaughan, Brian A.
Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
topic_facet Ciencias Astronómicas
Accretion, accretion disks
Stars: neutron
Stars: individual (4 U 1608–52)
X-rays: stars
description We present new Rossi X-ray Timing Explorer observations of the low-mass X-ray binary 4U 1608-52 during the decay of its 1998 outburst. We detect by a direct FFT method the existence of a second kilohertz quasi-periodic oscillation (kHz QPO) in its power density spectrum, previously only seen by means of the sensitivity-enhancing `shift and add' technique. This result confirms that 4U 1608-52 is a twin kHz QPO source. The frequency separation between these two QPO decreased significantly, from 325.5 +/- 3.4 Hz to 225.3 +/- 12.0 Hz, as the frequency of the lower kHz QPO increased from 470 Hz to 865 Hz, in contradiction with a simple beat-frequency interpretation. This change in the peak separation of the kHz QPOs is closely similar to that previously seen in Sco X-1, but takes place at a ten times lower average luminosity. We discuss this result within the framework of models that have been proposed for kHz QPO. Beat frequency models where the peak separation is identified with the neutron star spin rate, as well as the explanations previously proposed to account for the similar behavior of the QPOs in Sco X-1, are strongly challenged by this result.
format Articulo
Preprint
author Méndez, Mariano R.
van der Klis, Michiel
Wijnands, Rudy
Ford, Eric
van Paradijs, Jan
Vaughan, Brian A.
author_facet Méndez, Mariano R.
van der Klis, Michiel
Wijnands, Rudy
Ford, Eric
van Paradijs, Jan
Vaughan, Brian A.
author_sort Méndez, Mariano R.
title Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
title_short Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
title_full Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
title_fullStr Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
title_full_unstemmed Kilohertz Quasi-Periodic Oscillation Peak Separation is not Constant in the Atoll Source 4U 1608-52
title_sort kilohertz quasi-periodic oscillation peak separation is not constant in the atoll source 4u 1608-52
publishDate 1998
url http://sedici.unlp.edu.ar/handle/10915/123191
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