Recent phase changes in X Persei: optical, infrared and X-ray behaviour
We present a set of optical and IR photometric measurements which show the lightcurve of the Be/X-ray binary system X Persei over the last 25 yr. During this period, the Be star has undergone two extended faint, nonvariable phases, the last of which (1990-present) has been shown to be related to the...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 1993-03, Vol.270 (1-2), p.122-138 |
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Sprache: | eng |
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