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Zoology and wildlife conservation

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A long-period globular-cluster pulsar in an eclipsing binary system

Article Abstract:

Pulsar PSR1718-19 is an exception to the rule that pulsar members of eclipsing binary systems found in globular clusters rotate rapidly. It exhibits the relatively long period of 1 s, has a strong magnetic field and small spin-down age. Observations of the eclipses show that a cloud of material surrounds the binary system. This cloud was probably ejected from the companion, and this may have been caused by the pulsar's radiation. This shows that pulsars may have a greater influence on their binary companions than previously believed.

Author: Lyne, A.G., Bailes, M., Biggs, J.D., Harrison, P.A.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1993
Stars, Globular clusters (Astronomy)

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Pulsed X-rays from the Vela pulsar

Article Abstract:

The Rosat satellite has confirmed that the Vela pulsar, PSR0833-45, is a neutron star whose emissions of pulsed radiation include X-rays as well as the previously detected radio waves, optical light and gamma-rays. Rosat's data, collected in two sets in Apr and Dec 1991, also demonstrate the comparative softness of the pulsar's X-ray emissions. This soft radiation is similar to what 100,000-year-old pulsars produce, although PSR0833-45 itself is only about 10,000 years old.

Author: Ogelman, H., Finley, J.P., Zimmermann, H.U.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1993
Spectra, Neutron stars

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X-rays from the eclipsing pulsar 1957+20

Article Abstract:

The eclipsing pulsar PSR1957+20 is emitting soft X-rays of about 1 keV energy. This X-ray wind is apparently created as the pulsar eclipses a low-mass companion star. However, the details of this process remain mysterious. Three sources for the X-rays have been proposed: the interstellar nebula, the pulsar's interaction with its companion star and the pulsar itself. The small size of the X-ray producer indicates that the X-rays are generated within the binary system.

Author: Fruchter, A.S., Bookbinder, J., Garcia, M.R., Bailyn, C.D.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1992

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Subjects list: Observations, Pulsars, Eclipsing binaries, Research, X-ray astronomy
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