Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera

Details Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.8012b&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #80.12; Bulletin of the American Astronomical Society, Vol. 24, p.1251

Astronomy and Astrophysics

Astronomy

Scientific paper

The Wide Field Camera (WFC) on the ROSAT satellite conducted the first all-sky survey in the extreme ultraviolet (EUV) over the six month period beginning on 1990 July 30. Two survey filters were used peaking at 95 and 120 Angstroms . Many of the sources detected are coronal stars. We present detailed results from WFC survey data for a range of coronal stars, including a complete survey of the RS CVn systems in the Strassmeier catalog (40% detection rate), the EUV variability of the flare star EV Lac (including the largest flare seen by the WFC from a coronal source), the EUV rotation-activity relation for a homogeneous sample of single early K dwarfs, and WFC results forming part of the RIASS (ROSAT-IUE-All-Sky-Survey) campaign. This work is supported by NASA grant NAG 5-1792 to the University of Colorado.

Affiliated with

Also associated with

No associations

Rating

Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera 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 Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Coronal EUV Emission Observed with the ROSAT Wide Field Camera will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1111574