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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 |