Search Results - "Ge, M Y"
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Relation of Cyclotron Resonant Energy and Luminosity in a Strongly Magnetized Neutron Star GRO J1008-57 Observed by Insight-HXMT
Published in The Astrophysical journal (01-09-2021)“…Abstract Cyclotron line scattering features are detected in a few tens of X-ray pulsars (XRPs) and used as direct indicators of a strong magnetic field at the…”
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2
A Detailed View of Low-frequency Quasi-periodic Oscillation in the Broadband 0.2–200 keV with Insight-HXMT and NICER
Published in The Astrophysical journal (01-05-2023)“…Abstract We report the X-ray timing results of the black hole candidate MAXI J1820+070 during its 2018 outburst using the Hard X-ray Modulation Telescope…”
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3
Pulse profile variability associated with the glitch of PSR J1048-5832
Published in Monthly notices of the Royal Astronomical Society (01-10-2024)“…ABSTRACT PSR J1048$-$5832 (B1046$-$58) is a Vela-like pulsar that has exhibited multiple glitch events. In this study, we analyse the timing data spanning…”
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4
Insight-HXMT Views Her X-1: Probing the Dependence of the Cyclotron Line Energy on Flux and Time
Published in The Astrophysical journal (01-01-2024)“…Abstract Recent observations of Her X-1 with NuSTAR (as well as with INTEGRAL, Swift, and Astrosat) have provided evidence that the nearly 20 yr-long decay of…”
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5
Pulsed Iron Line Emission from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124
Published in The Astrophysical journal (01-04-2024)“…Abstract We report the phase-resolved spectral results of the first Galactic pulsating ultraluminous X-ray source (PULX) Swift J0243.6+6124, modeling its…”
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6
The braking index of PSR B0540−69 and the associated pulsar wind nebula emission after spin-down rate transition
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT In 2011 December, PSR B054−69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\…”
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7
Reanalysis of the X-Ray-burst-associated FRB 200428 with Insight-HXMT Observations
Published in The Astrophysical journal (01-08-2023)“…Abstract A double-peak X-ray burst from the Galactic magnetar SGR J1935+2154 was discovered to be associated with the two radio pulses of FRB 200428 separated…”
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8
Insight-HXMT Detections of Hard X-Ray Tails in Scorpius X-1
Published in The Astrophysical journal (01-06-2023)“…Abstract Using the observations of the high-energy detector of the Hard X-ray Modulation Telescope (Insight-HXMT) for Scorpius X-1 from 2017 to 2020, we search…”
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9
EVOLUTION OF THE X-RAY PROFILE OF THE CRAB PULSAR
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT Using the archival data from the Rossi X-ray Timing Explorer, we study the evolution of the Crab pulsar's X-ray profile in a time span of 11 years…”
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10
REVERSE-SHOCK IN TYCHO'S SUPERNOVA REMNANT
Published in The Astrophysical journal (01-06-2015)“…ABSTRACT Thermal X-ray emission from young supernova remnants (SNRs) is usually dominated by the emission lines of the supernova ejecta, which are widely…”
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11
Incorporating an immersed boundary method to study thermal effects of vascular systems during tissue cryo-freezing
Published in Journal of thermal biology (01-02-2017)“…In this paper, the three-dimensional thermal effects of a clinically-extracted vascular tissue undergoing cryo-freezing are numerically investigated. Based on…”
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12
Effect of Cadmium Exposure on the Histopathology of Cerebral Cortex in Juvenile Mice
Published in Biological trace element research (01-06-2015)“…Cadmium, a heavy metal, is a toxic environmental and industrial pollutant. Exposure to cadmium can lead to the toxic effects in a variety of tissues, also…”
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13
Glitches in four gamma-ray pulsars and inferences on the neutron star structure
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT We present timing solutions from the Fermi-LAT observations of gamma-ray pulsars PSR J0835 − 4510 (Vela), PSR J1023−5746, PSR J2111+4606, and PSR…”
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14
No pulsed radio emission during a bursting phase of a Galactic magnetar
Published in Nature (London) (05-11-2020)“…Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical origin observed at extragalactic distances 1 – 3 . It has long been…”
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15
Fan-beamed X-Ray Emission from 1 to above 130 keV from the Ultraluminous X-Ray Pulsar RX J0209.6-7427 in the Small Magellanic Cloud
Published in The Astrophysical journal (01-10-2022)“…Abstract We present detailed timing and spectral analyses of the transient X-ray pulsar RX J0209.6−7427 in the Small Magellanic Cloud during its 2019 giant…”
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16
Properties investigation on isotropical conductive adhesives filled with silver coated carbon nanotubes
Published in Composites science and technology (01-05-2007)“…In this study, chemical plating method was used to prepare silver coated carbon nanotubes (SCCNT). Fundamental materials characterizations including X-ray…”
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Timing Properties of the X-Ray Accreting Pulsar 1A 0535+262 Studied with Insight-HXMT
Published in The Astrophysical journal (01-08-2022)“…Abstract We report results on the timing analysis of the 2020 giant outburst of 1A 0535+262, using broadband data from Insight-HXMT. The analysis of the pulse…”
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18
Enhanced Localization of Transients Based on a Novel Cross-correlation Method
Published in The Astrophysical journal (01-10-2021)“…Abstract Locating gamma-ray transients including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts is of great importance in multi-messenger and…”
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19
High conductivity of isotropic conductive adhesives filled with silver nanowires
Published in International journal of adhesion and adhesives (01-12-2006)“…As an alternative to lead-bearing solder, isotropic conductive adhesives (ICA) have been utilized for many years in microelectronic packaging. In this study,…”
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New pulse profile variability associated with a glitch of PSR J0738-4042
Published in Monthly notices of the Royal Astronomical Society (01-02-2023)“…ABSTRACT The close correlation observed between emission state and spin-down rate change of pulsars has many implications both for the magnetospheric physics…”
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