Search Results - "DAL FIUME, D"
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Discovery of a Transient Absorption Edge in the X-ray Spectrum of GRB 990705
Published in Science (American Association for the Advancement of Science) (03-11-2000)“…We report the discovery of a transient equivalent hydrogen column density with an absorption edge at ∼3.8 kiloelectron volts in the spectrum of the prompt…”
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BEPPOSAX and Chandra Observations of SAX J0103.2–7209 = 2E 0101.5–7225: A New Persistent 345 Second X-Ray Pulsar in the Small Magellanic Cloud
Published in The Astrophysical journal (10-03-2000)“…We report the results of a 1998 July BeppoSAX observation of a field in the Small Magellanic Cloud which led to the discovery of approximately 345 s pulsations…”
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Discovery of an X-ray afterglow associated with the γ-ray burst of 28 February 1997
Published in Nature (London) (19-06-1997)“…Establishing the nature of γ-ray bursts is one of the greatest challenges in high-energy astrophysics. The distribution of these bursts is isotropic across the…”
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The broad band spectral properties of binary X-ray pulsars
Published in Advances in space research (2000)“…The X-ray telescopes on board BeppoSAX are an optimal set of instruments to observe bright galactic binary pulsars. These sources emit very hard and quite…”
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The Transient X-Ray Pulsar 4U 0115+63 from Quiescence to Outburst through the Centrifugal Transition
Published in The Astrophysical journal (10-11-2001)Get full text
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The X-Ray Afterglow of the Gamma-Ray Burst of 1997 May 8:Spectral Variability and Possible Evidence of an Iron Line
Published in The Astrophysical journal (01-04-1999)Get full text
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Broadband Spectrum of Cygnus X-1 in Two Spectral States with BeppoSAX
Published in The Astrophysical journal (10-01-2001)Get full text
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Hard X-Ray Emission from the Galaxy Cluster A2256
Published in The Astrophysical journal (01-05-2000)“…After the positive detection by BeppoSAX of hard X-ray radiation up to approximately 80 keV in the Coma Cluster spectrum, we present evidence for nonthermal…”
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BeppoSAX Observations of GRB 980425: Detection of the Prompt Event and Monitoring of the Error Box
Published in The Astrophysical journal (20-06-2000)Get full text
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A BEPPOSAX Study of the Pulsating Transient X0115+63: The First X-Ray Spectrum with Four Cyclotron Harmonic Features
Published in The Astrophysical journal (20-09-1999)Get full text
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BeppoSAX Observation of 4U 1626–67: Discovery of an AbsorptionCyclotron Resonance Feature
Published in The Astrophysical journal (20-06-1998)Get full text
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Spectral Properties of the Prompt X-ray Emission and Afterglow from the Gamma-Ray Burst of 1997 February 28
Published in The Astrophysical journal (01-02-1998)Get full text
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Prompt and Afterglow Emission from the X-Ray-Rich GRB 981226 Observed with BeppoSAX
Published in The Astrophysical journal (10-09-2000)Get full text
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Aquila X-1 from Outburst to Quiescence: The Onset of the Propeller Effect and Signs of a Turned-on Rotation-powered Pulsar
Published in The Astrophysical journal (20-05-1998)Get full text
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Integrating the BeppoSAX Gamma-Ray Burst Monitor into the Third Interplanetary Network
Published in The Astrophysical journal (01-05-2000)Get full text
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Radio Monitoring of the 1997 January 11 Gamma-Ray Burst
Published in The Astrophysical journal (10-07-1997)Get full text
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The Gamma-Ray Bursts Monitor onboard SAX
Published in Advances in space research (01-01-1998)“…The four Lateral Shields of the PDS experiment aboard the Beppo-SAX satellite are equipped with dedicated electronics and used as a Gamma Ray Burst Monitor…”
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BeppoSAX observations of an orbital cycle of the X-ray binary pulsar GX 301-2
Published in Advances in space research (2000)“…We present preliminary results on our campaign of observations of the X-ray binary pulsar GX301-2. BeppoSAX observed this source six times in January/February…”
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BeppoSAX observations of the massive X-ray pulsar Cen X-3: Broad-band spectra and iron line diagnostic
Published in Advances in space research (2000)“…The BeppoSAX satellite pointed to the massive X-ray pulsar Cen X-3 for the first time during the Science Verification Phase (SVP). The source was found in a…”
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