New observations of the cyclotron absorption feature in Hercules X-1

The Ginga satellite observatory has been used to measure a cyclotron feature in the hard X-ray spectrum of the 1.24-s binary pulsar Hercules X-1 with a much greater energy resolution than in previous observations. The spectrum from 10-60 keV can be described with a simple analytical formula which in...

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Veröffentlicht in:Nature (London) 1990-07, Vol.346 (6281), p.250-252
Hauptverfasser: Mihara, T., Makishima, K., Ohashi, T., Sakao, T., Tashiro, M.
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container_issue 6281
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container_title Nature (London)
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creator Mihara, T.
Makishima, K.
Ohashi, T.
Sakao, T.
Tashiro, M.
description The Ginga satellite observatory has been used to measure a cyclotron feature in the hard X-ray spectrum of the 1.24-s binary pulsar Hercules X-1 with a much greater energy resolution than in previous observations. The spectrum from 10-60 keV can be described with a simple analytical formula which indicates an absorption feature at about 34 keV rather than an emission feature at about 50 keV. From this, the surface magnetic field strength of Her X-1 is estimated to be (2.9 + or - 0.3) x 10 to the 12th G.
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source Nature; NASA Technical Reports Server; SpringerLink Journals - AutoHoldings
subjects Absorption
Astronomy
Astrophysics
Cyclotron resonance
Earth, ocean, space
Energy
Energy measurement
Energy resolution
Exact sciences and technology
Field strength
Humanities and Social Sciences
Late stages of stellar evolution (including black holes)
letter
Magnetic fields
multidisciplinary
Neutron stars
Pulsars
Satellite observation
Science
Science (multidisciplinary)
Stars
X-ray spectra
title New observations of the cyclotron absorption feature in Hercules X-1
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