Investigation of physical parameters in stellar flares observed by GINGA

Details Investigation of physical parameters in stellar flares observed by GINGA Investigation of physical parameters in stellar flares observed by GINGA

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994lock.reptr....s&link_type=abstract

Final Report, 20 Jul. 1993 - 19 Sep. 1994 Lockheed Missiles and Space Co., Palo Alto, CA.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Spectrum Analysis, Stellar Flares, Stellar Models, Stellar Radiation, X Ray Astronomy, X Ray Spectra, Ginga Satellite, Orbit Calculation, Stellar Luminosity

Scientific paper

This program involves analysis and interpretation of results from GINGA Large Area Counter (LAC) observations from a group of large stellar x-ray flares. All LAC data are re-extracted using the standard Hayashida method of LAC background subtraction and analyzed using various models available with the XSPEC spectral fitting program. Temperature-emission measure histories are available for a total of 5 flares observed by GINGA. These will be used to compare physical parameters of these flares with solar and stellar flare models.

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