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dc.date.accessioned 2021-08-19T19:18:35Z
dc.date.available 2021-08-19T19:18:35Z
dc.date.issued 1998-02-10
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/123023
dc.description.abstract 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. en
dc.format.extent 65-69 es
dc.language en es
dc.subject accretion, accretion disks es
dc.subject stars: neutron es
dc.subject stars: individual (4U 1608252) es
dc.subject X-rays: stars es
dc.title Discovery of a second kilohertz quasi-periodic oscillation peak in 4U 1608-52 en
dc.type Articulo es
sedici.identifier.other doi:10.1086/311162 es
sedici.identifier.issn 0004-637X es
sedici.creator.person Méndez, Mariano R. es
sedici.creator.person Klis, M. van der es
sedici.creator.person Paradijs, J. van es
sedici.creator.person Lewin, Walter H. G. es
sedici.creator.person Vaughan, Brian A. es
sedici.creator.person Kuulkers, Erik es
sedici.creator.person Zhang, W. W. es
sedici.creator.person Lamb, Frederick K. es
sedici.creator.person Psaltis, Dimitrios es
sedici.subject.materias Astronomía es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle The Astrophysical Journal es
sedici.relation.journalVolumeAndIssue vol. 494, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)