Extended Thermal X-Ray Emission from the Spiral-Dominant Group of Galaxies HCG 57

We observed a group of galaxies, HCG 57, with ASCA. Regardless that their member galaxies are dominated by spiral galaxies, we detected extended thermal X-ray emission that is attributed to hot gas with a temperature of 1.04 +/- 0.10 keV. This is the second clear detection of thermal X-ray emission from a spiral-dominant group of galaxies after HCG 92. The luminosity of the thermal emission is about 5 × 10⁴¹ erg s^-1 in the 0.5-10keV band, which is higher than that of HCG 92, but relatively less luminous among groups of galaxies. The X-ray emission is extended over several member galaxies, and is thus associated with the group rather than an individual galaxy. The metal abundance cannot be well constrained with a lower limit of 0.08 solar. The gas-to-stellar mass ratio is ~ 0.3. Although this is relatively low among groups, the hot gas is also a significant component even in the spiral-dominant group. We suggest that the X! ! -ray faintness of spiral-dominant groups is due to the low surface brightness and somewhat low gas mass, at least in the case of HCG 57.