Correlations Between the Flaring Radio Emission and Starspot Distribution of UX Arietis.

We have observed UX Arietis at C band (6 cm) for 3 weeks with four Very Long Array (VLA) antennas. The temporal coverage during the program was approximately three scans per day. A few days into the VLA program, UX Ari began a radio flaring period which lasted for at least 2 weeks. All the radio flu...

Bibliographic Details
Main Authors:	Elias II, Nicholas M., Quirrenbach, Andreas., Witzel, Arno., Naundorf, Christian E., Wegner, Ralf., Guinan, Edward F., McCook, George P.
Format:	Villanova Faculty Authorship
Language:	English
Published:	1994
Online Access:	http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176505

Main Authors:

Elias II, Nicholas M., Quirrenbach, Andreas., Witzel, Arno., Naundorf, Christian E., Wegner, Ralf., Guinan, Edward F., McCook, George P.

Format:

Villanova Faculty Authorship

Language:

English

Published:

1994

Online Access:

http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176505

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Correlations Between the Flaring Radio Emission and Starspot Distribution of UX Arietis.

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