Astro-D observations of flares: Detecting the impulsive phase

Details Astro-D observations of flares: Detecting the impulsive phase Astro-D observations of flares: Detecting the impulsive phase

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995lock.rept.....h&link_type=abstract

Final Report, 20 Apr. 1994 - 15 Oct. 1995 Lockheed Martin Palo Alto Research Lab., Palo Alto, CA.

Astronomy and Astrophysics

Astronomy

Centaurus Constellation, Flare Stars, Solar X-Rays, Stellar Systems, X Ray Astronomy, Astronomical Observatories, Detection, Stellar Structure

Scientific paper

The flare star Proxima Centauri was observed by the satellite for approximately 50 ks and a number of flares were successfully detected. The scientific results were presented at several meetings and were discussed in articles, primarily in 'Solar-like M-Class X-ray Flares on Proxima Centauri Observed by the ASCA Satellite' by Haisch, Antunes and Schmitt, Science, Vol. 268, pp. 1327-1329, attached to the report.

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