Flare-related color effects in UV Ceti stars

Details Flare-related color effects in UV Ceti stars Flare-related color effects in UV Ceti stars

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phdt.........4f&link_type=abstract

Ph.D. Thesis Florida Univ., Gainesville.

Physics

1

Color, Line Spectra, Photoelectricity, Stars, Ultraviolet Spectra, Solar Flares, Solar Spectra, Telescopes

Scientific paper

The UV Ceti flare stars YZ CMi, BD+16 deg 2708, EV Lac, and AD Leo were monitored photoelectrically for flare activity with the 76 centimeter reflecting telescope of the University of Florida's Rosemary Hill Observatory. Observations were carried out from January, 1973 to April, 1975. The instrumentation allowed simultaneous readings to be taken at 3500, 4632, and 6496 A with a time resolution of 2 seconds. A total of 15 major events were observed, with 14 of these being observed in all three colors. All events showed the classical fast rise and slower decline that is typical of this type of activity. One event showed peculiar behavior in the red bandpass that may indicate strong dependence of the flare light in some cases on line emission.

Affiliated with

Also associated with

No associations

Rating

Flare-related color effects in UV Ceti stars 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 Flare-related color effects in UV Ceti stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flare-related color effects in UV Ceti stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1000252