An X ray pulsar in the dark cloud LYNDS 1457

Details An X ray pulsar in the dark cloud LYNDS 1457 An X ray pulsar in the dark cloud LYNDS 1457

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296...99k&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 99-101(SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Dark Matter, Molecular Clouds, Pulsars, X Ray Spectra, Interstellar Gas, White Dwarf Stars, X Ray Astronomy, X Ray Binaries

Scientific paper

An X-ray pulsar was discovered in the center of the dark cloud Lynds
1457. The nature of the X-ray pulsar is discussed. It is a binary X-ray
pulsar or a collapse star in the dense gas. The age of the dark cloud is
estimated to be about 100,000 years, the presence of a neutron star or
white dwarf in the dark cloud is discussed.

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