Search Results - "Day, S.R."
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Characterization and Cloning of the Cathepsin L Proteinases of Schistosoma japonicum
Published in Biochemical and biophysical research communications (05-12-1995)“…Adult Schistosoma japonicum parasites synthesize and secrete both cathepsin L and cathepsin B cysteine proteinases. The specific activities of cathepsin L were…”
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ASCA and GRO Observations of GX 301-2
Published in The Astrophysical journal (01-12-1995)Get full text
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3
X-Ray Spectroscopy of Centaurus X-3 with ASCA over an Eclipse
Published in Publications of the Astronomical Society of Japan (01-06-1996)“…The X-ray binary pulsar Cen X-3 was observed with the ASCA satellite over an entire binary eclipse. With unprecedented energy resolution at the iron K-energy…”
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4
Pulse Phase-Dependent Spectroscopic Study of Vela X-1
Published in The Astrophysical journal (01-11-1996)“…Abstract only…”
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5
An ASCA Observation of the X-Ray Binary GX 301-2
Published in The Astrophysical journal (01-06-1996)Get full text
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6
GINGA observations of the Shapley Supercluster
Published in Monthly notices of the Royal Astronomical Society (01-10-1991)“…We present the results of scanning and pointed X-ray observations of a region of about 40 square degrees in the vicinity of the rich cluster Shapley 8, in the…”
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A disc-reflected component in the spectra of X-ray bursters
Published in Monthly notices of the Royal Astronomical Society (01-11-1991)“…We show that a disc-reflection component, as seen in AGN, can be detected in the spectrum of X-ray bursts during the burst tail, and speculate on the use of…”
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Dust scattering in the high-state eclipse of Cen X-3
Published in Monthly notices of the Royal Astronomical Society (01-07-1991)“…EXOSAT data from two high-state eclipses of Cen X-3 are analysed for the effects of dust scattering. The light curves show bright (2 per cent of the…”
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A search for the iron absorption edge in the tail of an X-ray burst from X1636–53
Published in Monthly notices of the Royal Astronomical Society (01-08-1992)“…Model atmosphere calculations of the spectrum of a neutron star cooling after an X-ray burst show that the photoelectric edge of iron should be prominent. We…”
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