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An IUE survey of activity in red giants and supergiants

  • I. Oznovich
  • D. M. Gibson
Session I: Dynamos and Stellar Activity: Observations
Part of the Lecture Notes in Physics book series (LNP, volume 254)

Abstract

We examine chromospheric and transition region line activity in apparently single red giants and supergiants using the ME archives. Low resolution, large aperture spectra (mostly short-wavelength ones) were used to search for variations of emission line fluxes in time. We implemented a series of automatic processing procedures in order to uniformly calibrate a large number of spectra, fit continua to each of them, determine the fluxes of as many as 18 emission lines and compare them at different epochs. A method to compute the overall error in the integrated flux (being the crucial activity measure used) independent of the observing and processing details is offered. The data-base consisted of ∼120 images taken over a period of seven years. We detected UV emission line flux variations in four stars, comprising 15% of the tracked stellar set. All four stars lie in a region of the HR diagram in which time-dependent circumstellar absorption lines appear.

Keywords

Emission Line Line Flux Hybrid Star Standard Calibration Procedure Variability Magnitude 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Ayres 1985, personal communication.Google Scholar
  2. Bohlin, R.C. and Holm, A. 1980, IUE NASA Newsletter, no. 10, p. 37.Google Scholar
  3. Cassatella, A., Holm, A., Ponz, D. and Schiffer, F.H. 1980, IUE NASA Newsletter, no. 8, p. 1.Google Scholar
  4. Cassinelli, J. et al. 1983, Ap.J. 268 205.CrossRefGoogle Scholar
  5. Reimers, D. 1977, Astron. Astrophys. 57, 395.Google Scholar

Copyright information

© Springer-Verlag 1986

Authors and Affiliations

  • I. Oznovich
  • D. M. Gibson

There are no affiliations available

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