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相关论文: The 1999 Hercules X-1 Anomalous Low State

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We searched for coherent X-ray pulsations from Aql X-1 in a series of RXTE observations taken shortly after a recent outburst. During the course of these observations, Aql X-1 passes through an apparent ``propeller'' phase as its luminosity…

天体物理学 · 物理学 2009-10-31 A. M. Chandler , R. E. Rutledge

First results of observations of the low mass X-ray binary Her X-1/HZ Her performed by the INTEGRAL satellite in July-August 2005 are presented. A significant part of one 35 day main-on state was covered. The cyclotron line in the X-ray…

A statistical analysis of the space-time distribution of absorption-line systems (ALSs) observed in QSO spectra within the cosmological redshift interval $z$=0.0--3.7 is carried out on the base of our catalog of absorption systems…

天体物理学 · 物理学 2008-11-26 A. I. Ryabinkov , A. D. Kaminker , D. A. Varshalovich

We present 12 observations of the accreting millisecond X-ray pulsar Aql X-1, taken from August 2022 to October 2023 using the Five-hundred-meter Aperture Spherical Radio Telescope at 1250 MHz. These observations covered both the quiescence…

高能天体物理现象 · 物理学 2025-04-22 Long Peng , Zhaosheng Li , Yuanyue Pan , Shanshan Weng , Wengming Yan , Na Wang , Bojun Wang , Shuangqiang Wang

The X-ray pulsar GX 1+4 was observed with the RXTE satellite for a total of 51ks between 1996 July 19 - 21. During this period the flux decreased smoothly from an initial mean level of ~ 6 X 10^36 erg/s to a minimum of ~ 4 X 10^35 erg/s…

天体物理学 · 物理学 2016-08-30 D. K. Galloway , A. B. Giles , J. G. Greenhill , M. C. Storey

We find line emission from the hydrogen- and/or helium-like ions of Ne, O, N and C in the low and short-on states of Her X-1, using the XMM-Newton Reflection Grating Spectrometer. The emission line velocity broadening is 200 < sigma < 500…

天体物理学 · 物理学 2007-05-23 M. A. Jimenez-Garate , C. J. Hailey , J. W. den Herder , S. Zane , G. Ramsay

We present results from a 20 h RXTE observation of Vela X-1, ncluding a peculiar low state of a few hours duration, during which the pulsation of the X-ray emission ceased, while significant non-pulsed emission remained. This ``quiescent…

天体物理学 · 物理学 2009-10-31 P. Kretschmar , I. Kreykenbohm , J. Wilms , R. Staubert , W. A. Heindl , D. E. Gruber , R. E. Rothschild

When accretion temporarily ceases in the polar AM Her, the emission line profiles are known to develop several distinct components, whose origin remains poorly understood. The new low-state spectra reported here have a more favorable…

天体物理学 · 物理学 2009-11-13 S. Kafka , T. Ribeiro , R. Baptista , R. K. Honeycutt , J. W. Robertson

We report on the spectral analysis of Circinus X-1 observed by the ASCA satellite in March 1998 along one orbital period. The luminosity of the source (in the 0.1-100 keV band) ranges from $2.5 \times 10^{38}$ erg s$^{-1}$ at the periastron…

天体物理学 · 物理学 2009-11-06 R. Iaria , T. Di Salvo , L. Burderi , N. R. Robba

We report BeppoSAX and optical observations of the black hole candidate GX 339-4 during its X-ray `off' state in 1999. The broad-band (0.8-50 keV) X-ray emission can be fitted by a single power law with spectral index, \alpha ~1.6. The…

天体物理学 · 物理学 2009-10-31 A. K. H. Kong , E. Kuulkers , P. A. Charles , L. Homer

We present orbit-resolved spectroscopic and photometric observations of the polar ST LMi during its recent low and high states. In the low state spectra, we report the presence of blue and red satellites to the H-alpha emission line; the…

天体物理学 · 物理学 2008-11-26 S. Kafka , S. B. Howell , R. K. Honeycutt , J. W. Robertson

Her X-1 is one of the the most intensively studied Accreting X-ray Binary Pulsars (AXBPs). This is largely because it is a bright and persistent X-ray pulsar, showing the largest variety of observable phenomena, partly due to the favorable…

高能天体物理现象 · 物理学 2013-03-15 Ruediger Staubert

Frequency glitches have been observed so far only in radio pulsars and anomalous X-ray pulsars. Here we present evidence of a glitch in a neutron star accreting from a Be companion. The transient KS 1947+300 reappeared in 2000 October as a…

天体物理学 · 物理学 2009-11-10 D. K. Galloway , E. H. Morgan , A. M. Levine

X-ray binary accretion disk winds can carry away a significant fraction of the matter transferred from the companion and hence strongly affect the accretion flow and the long-term evolution of the binary. However, accurate mass outflow rate…

Accretion of matter onto the surface of a freely precessing NS with a complex non-dipole magnetic field can explain the change of X-ray pulse profiles of Her X-1 observed by RXTE with the phase of the 35-day cycle. We demonstrate this using…

高能天体物理现象 · 物理学 2013-07-25 K. Postnov , N. Shakura , . R. Staubert , A. Kochetkova , D. Klochkov , J. Wilms

We present the results of a detailed analysis of RXTE observations of class $\omega$ which show an unusual state transition between high-soft and low-soft states in the microquasar GRS 1915+105. Out of about 600 pointed RXTE observations,…

天体物理学 · 物理学 2009-11-07 S. Naik , A. R. Rao , Sandip K. Chakrabarti

We conduct a comprehensive analysis of the accreting X-ray pulsar, Hercules X-1, utilizing data from IXPE and NuSTAR. IXPE performed five observations of Her X-1, consisting of three in the Main-on state and two in the Short-on state. Our…

We report on a spectral-timing analysis of the neutron star low-mass X-ray binary Aql~X-1 with the Neutron Star Interior Composition Explorer (NICER) on the International Space Station. Aql~X-1 was observed with NICER during a dim outburst…

We present temporal and spectral results from monitoring Cygnus X-1 with the Rossi X-ray Timing Explorer (RXTE) in 1998 and 1999. We concentrate on the long term evolution of the hard state timing properties, comparing it to the 1996 soft…

天体物理学 · 物理学 2009-10-31 K. Pottschmidt , J. Wilms , R. Staubert , M. A. Nowak , W. A. Heindl , D. M. Smith