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UV time-dependent emission in SY Muscae

Published online by Cambridge University Press:  12 April 2016

A.G. Michalitsianos
Affiliation:
NASA Goddard Space Flight Center, Greehbelt, Md. 20771 USA
M. Kafatos
Affiliation:
George Mason University, Department of Physics Fairfax, Virginia 22030, USA

Extract

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Ultraviolet spectra acquired with the International Ultraviolet Explorer (IUE) of SY Mus = HD 10036 on 20 September 1980 and 11 June 1981 indicate a substantial enhancement of UV emission over a nine month period. The general UV flux level appears to have increased by approximately one order of magnitude between the first and second observing epochs. The strong ultraviolet continuum evident throughout the entire IUE spectral range λλ1200-3200 A on 11 June 1981 is closely approximated by a star with Teff = 40,000 K, where previously on 20 September 1980 the continuum distribution presented a more complex structure that is possibly explained by a combination of thermal emission from an early type main sequence star, and nebular recombination emission (Michalitsianos et al. 1981).

Type
Session II – Discussion on Individual Stars
Copyright
Copyright © Reidel 1982

References

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