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Related papers: The atoll source 4U 1608-52 is not a Z source

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The X-ray burster and dipper 4U1915-05 (also known as XB1916-053) was observed 19 times for a total exposure of roughly 140 ks between 1996 February and October with the proportional counter array (PCA) aboard Rossi X-ray Timing Explorer…

Astrophysics · Physics 2007-05-23 L. Boirin , D. Barret , J. F. Olive , P. F. Bloser , J. E. Grindlay

In this work we investigate broad band (1-79 keV) spectral nature of the atoll source 4U 1636-536 using the combined Nu-STAR and SWIFT-XRT data. The spectra are complex and have emission components from the disc, boundary-layer and corona.…

High Energy Astrophysical Phenomena · Physics 2016-11-29 Vivek Kumar Agrawal , Mohammad Hasan

We study the timing properties of the bursting atoll source 4U 1728-34 as a function of its position in the X-ray color-color diagram. In the island part of the color-color diagram (corresponding to the hardest energy spectra) the power…

Astrophysics · Physics 2009-10-31 T. Di Salvo , M. Méndez , M. van der Klis , E. Ford , N. R. Robba

We report on about 4 hrs of observations made with the Rossi X-ray Timing Explorer on 1997 May 2 of the low-mass X-ray binary and Z source GX 349+2 (Sco X-2). Initially the source was in the normal branch (NB), later it moved to the flaring…

Astrophysics · Physics 2007-05-23 Erik Kuulkers , Michiel van der Klis

Using archival RXTE data we derive the 2-16 keV Fourier-resolved spectra of the Atoll source 4U 1728-34 in a sequence of its timing states as its low QPO frequency spans the range between 6 and 94 Hz. The increase in the QPO frequency…

Astrophysics · Physics 2009-11-13 C. R. Shrader , P. Reig , D. Kazanas

We studied the aperiodic X-ray timing behaviour of the accreting millisecond pulsar SAX J1808.4-3658. The source was recently found to be the first accreting millisecond pulsar that shows the kilohertz quasi-periodic oscillations (kilohertz…

Astrophysics · Physics 2009-11-10 S. van Straaten , M. van der Klis , R. Wijnands

We present the spectro-polarimetric results obtained from simultaneous X-ray observations with IXPE, NuSTAR and NICER of the dipping neutron star X-ray binary 4U 1624-49. This source is the most polarized Atoll source so far observed with…

High Energy Astrophysical Phenomena · Physics 2024-10-16 Andrea Gnarini , M. Lynne Saade , Francesco Ursini , Stefano Bianchi , Fiamma Capitanio , Philip Kaaret , Giorgio Matt , Juri Poutanen , Wenda Zhang

We have re-analyzed two EXOSAT Medium Energy observations during part of the 1984 X-ray outburst of the black-hole candidate transient system 4U 1630-47. One observation (May 10) shows fast timing properties (on timescales shorter than ~250…

Astrophysics · Physics 2009-10-28 Erik Kuulkers , Michiel van der Klis , Arvind N. Parmar

Exploiting the presence of kilohertz quasi-periodic oscillations (QPOs) in the timing power spectrum, we find that the soft x-ray emission of the neutron-star X-ray binary and atoll source 4U1636-536 modulated at the QPO frequency lags…

Astrophysics · Physics 2009-10-31 Philip Kaaret , Santina Piraino , Eric C. Ford , Andrea Santangelo

We present an analysis of the RXTE observations of 4U 1630-47 during its outburst of 1998. The light curve and the spectral evolution of the outburst were distinctly different from the outbursts of the same source in 1996 and in 1999.…

We report three RXTE/PCA observations of the low-mass X-ray binary 4U 0614+09. They show strong (~ 30% rms) band-limited noise with a cut-off frequency varying between 0.7 and 15 Hz in correlation with the X-ray flux. We observe two…

Spectral state transitions in neutron star LMXB systems have been widely observed yet not well understood. Here we report an abrupt spectral change in 4U 1608-52, a typical atoll source, during its decay phase of the 2004 outburst. The…

Astrophysics · Physics 2010-11-11 Xie Chen , Shuang Nan Zhang , Guo Qiang Ding

We report on the evolution of the timing of 4U1630-47 during its 1998 outburst using data obtained with the Rossi X-ray Timing Explorer (RXTE). The count rate and position in hardness-intensity, color-color diagrams and simple spectral fits…

It is known that the Z and atoll sources are two typical types of neutron-star sources in low mass X-ray binaries (LMXBs), which present very different Q-$\nu$ relations of lower kHz QPOs. We propose that the Z and atoll sources are two…

High Energy Astrophysical Phenomena · Physics 2015-06-12 J. Wang , H. -K. Chang

We detect millihertz quasi-periodic oscillations (mHz QPOs) using the Rossi X-ray Time Explorer (RXTE) from the atoll neutron-star (NS) low-mass X-ray binaries 4U 1608--52 and Aql X--1. From the analysis of all RXTE observations of 4U…

High Energy Astrophysical Phenomena · Physics 2021-02-03 G. C. Mancuso , D. Altamirano , M. Méndez , M. Lyu , J. A. Combi

A long discussion has been devoted to the issue of clustering of the kHz QPO frequency ratios in the neutron star sources. While the distribution of ratios inferred from an occurrence of a single QPO seems to be consistent with a random…

We report results from the spectro-timing analysis of the atoll source 4U 1636$-$536 observed with NuSTAR and AstroSat during its hard spectral state. In three observations of 207 ks total exposure, we identify 31 thermonuclear X-ray bursts…

High Energy Astrophysical Phenomena · Physics 2022-08-03 Pinaki Roy , Aru Beri , Aditya S. Mondal

We present a spectral and timing analysis of INTEGRAL observations of two high mass X-ray binaries, 4U 1538-522 and 4U 1907+09. Our timing measurements for 4U 1538-522 find the pulse period to have exhibited a spin-up trend until…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Paul Hemphill , Richard Rothschild , Isabel Caballero , Katja Pottschmidt , Matthias Kuehnel , Felix Fuerst , Joern Wilms

We analyze archival Rossi X-ray Timing Explorer (RXTE) Proportional Counter Array (PCA) data of the low mass X-ray binary (LMXB) system XB 1254-690. We calculate colour-colour diagram, hardness-intensity diagram and power spectra of this…

Astrophysics · Physics 2008-11-26 Sudip Bhattacharyya

We analysed 14 observations with kilohertz quasi-periodic oscillations (kHz QPOs) of the neutron star X-ray binary XTE J1701$-$462, the first source to show a clear transition between atoll and Z-like behaviour during a single outburst. We…

High Energy Astrophysical Phenomena · Physics 2022-04-27 Valentina Peirano , Mariano Méndez