Relations between timing features and colors in the X-ray binary 4U 0614+09

We study the correlations between timing and X-ray spectral properties in the low mass X-ray binary 4U 0614+09 using a large (265-ks) data set obtained with the Rossi X-ray Timing Explorer. We find strong quasi-periodic oscillations (QPOs) of the X-ray flux, like the kilohertz QPOs in many other X-r...

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Autores principales: van Straaten, Steve, Ford, Eric, van der Klis, Michiel, Méndez, Mariano R., Kaaret, Philip
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2000
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/127812
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id I19-R120-10915-127812
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
Black holes
Stars: individual (4U 0614+09)
Stars: neutron
X–rays: stars
spellingShingle Ciencias Astronómicas
Accretion
Accretion disks
Black holes
Stars: individual (4U 0614+09)
Stars: neutron
X–rays: stars
van Straaten, Steve
Ford, Eric
van der Klis, Michiel
Méndez, Mariano R.
Kaaret, Philip
Relations between timing features and colors in the X-ray binary 4U 0614+09
topic_facet Ciencias Astronómicas
Accretion
Accretion disks
Black holes
Stars: individual (4U 0614+09)
Stars: neutron
X–rays: stars
description We study the correlations between timing and X-ray spectral properties in the low mass X-ray binary 4U 0614+09 using a large (265-ks) data set obtained with the Rossi X-ray Timing Explorer. We find strong quasi-periodic oscillations (QPOs) of the X-ray flux, like the kilohertz QPOs in many other X-ray binaries with accreting neutron stars, with frequencies ranging from 1329 Hz down to 418 Hz and, perhaps, as low as 153 Hz. We report the highest frequency QPO yet from any low mass X-ray binary at 1329+-4 Hz, which has implications for neutron star structure. This QPO has a 3.5-sigma single-trial significance, for an estimated 40 trials the significance is 2.4-sigma. Besides the kilohertz QPOs, the Fourier power spectra show four additional components: high frequency noise (HFN), described by a broken power-law with a break frequency between 0.7 and 45 Hz, very low frequency noise (VLFN), which is fitted as a power-law below 1 Hz, and two broad Lorentzians with centroid frequencies varying from 6 to 38 Hz and 97 to 158 Hz, respectively. We find strong correlations between the frequencies of the kilohertz QPOs, the frequency of the 6 to 38 Hz broad Lorentzian, the break frequency of the HFN, the strength of both the HFN and the VLFN and the position of the source in the hard X-ray color vs. intensity diagram. The frequency of the 97 to 158 Hz Lorentzian does not correlate with these parameters. We also find that the relation between power density and break frequency of the HFN is similar to that established for black hole candidates in the low state. We suggest that the changing mass accretion rate is responsible for the correlated changes in all these parameters.
format Articulo
Preprint
author van Straaten, Steve
Ford, Eric
van der Klis, Michiel
Méndez, Mariano R.
Kaaret, Philip
author_facet van Straaten, Steve
Ford, Eric
van der Klis, Michiel
Méndez, Mariano R.
Kaaret, Philip
author_sort van Straaten, Steve
title Relations between timing features and colors in the X-ray binary 4U 0614+09
title_short Relations between timing features and colors in the X-ray binary 4U 0614+09
title_full Relations between timing features and colors in the X-ray binary 4U 0614+09
title_fullStr Relations between timing features and colors in the X-ray binary 4U 0614+09
title_full_unstemmed Relations between timing features and colors in the X-ray binary 4U 0614+09
title_sort relations between timing features and colors in the x-ray binary 4u 0614+09
publishDate 2000
url http://sedici.unlp.edu.ar/handle/10915/127812
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