Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-19T04:57:29.794Z Has data issue: false hasContentIssue false

VLBA Imaging of UX Ari

Published online by Cambridge University Press:  12 April 2016

A. J. Beasley
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
T.S. Bastian
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have used the Very Long Baseline Array (VLBA) and the Very Large Array (VLA) to perform multi-wavelength radio imaging of the RS CVn active binary UX Arietis during the period November 16–21 1995. A series of strong flaring events exhibiting optically-thick spectra peaking above 100 GHz and extended source structures consistent with inter-binary emission were detected.

Type
Research Article
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Carlos, R.C., & Popper, D.M. 1971. PASP, 83, 504507.CrossRefGoogle Scholar
Chiuderi-Drago, F., & Franciosini, E. 1993. ApJ, 410, 301308.CrossRefGoogle Scholar
Hall, D.S. 1976. IAU Colloq. 29, Multiple Periodic Variable Stars, ed. Fitch, W.S. (Dordrecht: Reidel), pp. 287290.Google Scholar
Mutel, R.L., et al. 1985. ApJ, 289, 262268.CrossRefGoogle Scholar
Tsuru, T., et al. 1989. PASJ, 41, 679695.Google Scholar
Uchida, Y., & Sakurai, T. 1983. Activity in Red Dwarf Stars, ed. Byrne, P.B., & Rodono, M. (Dordrecht: Reidel), 629632.Google Scholar
van den Oord, G.H.J., et al. 1988. A&A, 205, 181196.Google Scholar