The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari

Details The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.0802s&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #08.02; Bulletin of the American Astronomical Society, Vol. 34, p.653

Astronomy and Astrophysics

Astronomy

Scientific paper

We have studied the long-term behavior of radio flares from three binary systems: V711 Tau, β Per and UX Ari. The radio flares were collected with the Green Bank Interferometer continuously from 1995 to 2000 at frequencies of 2.3 GHz and 8.3 GHz (see Richards, Waltman, and Ghigo, these proceedings). Many strong flares were detected from the three systems. We found that flaring activity in β Per was nearly continuous, while V711 Tau and UX Ari were usually quiescent for 50 - 100 days before a large flare event. Long-term monitoring permitted us to discover both active and quiescent flaring epochs in V711 Tau and β Per which apparently last for more than 500 days in both systems. This work was supported by NSF grant AST-0074586.

Affiliated with

Also associated with

No associations

Rating

The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Long-term Characteristics of Radio Flares from V711 Tau, β Per and UX Ari will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1717223