Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52
- Autores
- Méndez, Mariano R.; Klis, M. van der; Paradijs, J. van; Lewin, Walter H. G.; Vaughan, Brian A.; Kuulkers, Erik; Zhang, W. W.; Lamb, Frederick K.; Psaltis, Dimitrios
- Año de publicación
- 1998
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Using a new technique to improve the sensitivity to weak quasi-periodic oscillations (QPOs), we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~600-900 Hz peak previously reported from these data. The frequency separation between the upper and the lower QPO peaks varied significantly from 232.7±11.5 Hz on March 3 to 293.1±6.6 Hz on March 6. This is the first case of a variable kilohertz peak separation in an atoll source. We discuss to what extent this result could be accommodated in beat-frequency models such as proposed for the kilohertz QPOs. We measured the rms fractional amplitude of both QPOs as a function of energy, and we found that the relation is steeper for the lower than for the upper frequency peak. This is the first source where such a difference between the energy spectrum of the two kilohertz QPOs could be measured.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Astronomía
Física
accretion, accretion disks
stars: neutron
stars: individual (4U 1608252)
X-rays: stars - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/123023
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Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52Méndez, Mariano R.Klis, M. van derParadijs, J. vanLewin, Walter H. G.Vaughan, Brian A.Kuulkers, ErikZhang, W. W.Lamb, Frederick K.Psaltis, DimitriosAstronomíaFísicaaccretion, accretion disksstars: neutronstars: individual (4U 1608252)X-rays: starsUsing a new technique to improve the sensitivity to weak quasi-periodic oscillations (QPOs), we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~600-900 Hz peak previously reported from these data. The frequency separation between the upper and the lower QPO peaks varied significantly from 232.7±11.5 Hz on March 3 to 293.1±6.6 Hz on March 6. This is the first case of a variable kilohertz peak separation in an atoll source. We discuss to what extent this result could be accommodated in beat-frequency models such as proposed for the kilohertz QPOs. We measured the rms fractional amplitude of both QPOs as a function of energy, and we found that the relation is steeper for the lower than for the upper frequency peak. This is the first source where such a difference between the energy spectrum of the two kilohertz QPOs could be measured.Facultad de Ciencias Astronómicas y Geofísicas1998-02-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf65-69http://sedici.unlp.edu.ar/handle/10915/123023enginfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/311162info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:10:09Zoai:sedici.unlp.edu.ar:10915/123023Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:10.233SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| title |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| spellingShingle |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 Méndez, Mariano R. Astronomía Física accretion, accretion disks stars: neutron stars: individual (4U 1608252) X-rays: stars |
| title_short |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| title_full |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| title_fullStr |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| title_full_unstemmed |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| title_sort |
Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 |
| dc.creator.none.fl_str_mv |
Méndez, Mariano R. Klis, M. van der Paradijs, J. van Lewin, Walter H. G. Vaughan, Brian A. Kuulkers, Erik Zhang, W. W. Lamb, Frederick K. Psaltis, Dimitrios |
| author |
Méndez, Mariano R. |
| author_facet |
Méndez, Mariano R. Klis, M. van der Paradijs, J. van Lewin, Walter H. G. Vaughan, Brian A. Kuulkers, Erik Zhang, W. W. Lamb, Frederick K. Psaltis, Dimitrios |
| author_role |
author |
| author2 |
Klis, M. van der Paradijs, J. van Lewin, Walter H. G. Vaughan, Brian A. Kuulkers, Erik Zhang, W. W. Lamb, Frederick K. Psaltis, Dimitrios |
| author2_role |
author author author author author author author author |
| dc.subject.none.fl_str_mv |
Astronomía Física accretion, accretion disks stars: neutron stars: individual (4U 1608252) X-rays: stars |
| topic |
Astronomía Física accretion, accretion disks stars: neutron stars: individual (4U 1608252) X-rays: stars |
| dc.description.none.fl_txt_mv |
Using a new technique to improve the sensitivity to weak quasi-periodic oscillations (QPOs), we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~600-900 Hz peak previously reported from these data. The frequency separation between the upper and the lower QPO peaks varied significantly from 232.7±11.5 Hz on March 3 to 293.1±6.6 Hz on March 6. This is the first case of a variable kilohertz peak separation in an atoll source. We discuss to what extent this result could be accommodated in beat-frequency models such as proposed for the kilohertz QPOs. We measured the rms fractional amplitude of both QPOs as a function of energy, and we found that the relation is steeper for the lower than for the upper frequency peak. This is the first source where such a difference between the energy spectrum of the two kilohertz QPOs could be measured. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Using a new technique to improve the sensitivity to weak quasi-periodic oscillations (QPOs), we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~600-900 Hz peak previously reported from these data. The frequency separation between the upper and the lower QPO peaks varied significantly from 232.7±11.5 Hz on March 3 to 293.1±6.6 Hz on March 6. This is the first case of a variable kilohertz peak separation in an atoll source. We discuss to what extent this result could be accommodated in beat-frequency models such as proposed for the kilohertz QPOs. We measured the rms fractional amplitude of both QPOs as a function of energy, and we found that the relation is steeper for the lower than for the upper frequency peak. This is the first source where such a difference between the energy spectrum of the two kilohertz QPOs could be measured. |
| publishDate |
1998 |
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1998-02-10 |
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