Optical and ultraviolet line and continuum emission from the Large Magellanic Cloud X-ray Be star A0538-66

Details Optical and ultraviolet line and continuum emission from the Large Magellanic Cloud X-ray Be star A0538-66 Optical and ultraviolet line and continuum emission from the Large Magellanic Cloud X-ray Be star A0538-66

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...335..147a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 335, Dec. 1, 1988, p. 147-149.

Astronomy and Astrophysics

Astronomy

3

B Stars, Continuous Radiation, Magellanic Clouds, Stellar Models, X Ray Binaries, Neutron Stars, Stellar Flares, Stellar Luminosity, Ultraviolet Astronomy, Visible Spectrum

Scientific paper

The X-ray Be star object A0538-66 in the LMC is a binary with a neutron
star emitting X-rays in flares when active. It is shown that the
enhanced continuum and line emission in the optical and ultraviolet is
from the ionized region formed by the X-rays in the gas ring around the
Be star.

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