ASCA observation of the NGC 2300 group of galaxies

Details ASCA observation of the NGC 2300 group of galaxies ASCA observation of the NGC 2300 group of galaxies

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..336..268t&link_type=abstract

Dark matter. AIP Conference Proceedings, Volume 336, pp. 268-271 (1995).

Computer Science

Performance

3

X-Ray, Small And Compact Galaxy Groups

Scientific paper

We report on NGC 2300 Group of galaxies observed with ASCA in the performance verification (PV) phase. Extended diffuse X-ray emission surrounded this galaxy group, which is first reported by ROSAT observation, was confirmed with its total luminosity of 4×1043 erg s-1 in the 0.6-2.6 keV band. We also found that the temperature of this hot gas was 0.90+/-0.14 keV and its elemental abundance was 0.09+/-0.05 of the solar value in the 90% confidence, if we adopt the thermal emission model derived by Raymond and Smith.

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