XMM-newton detects a hot gaseous halo in the fastest rotating spiral galaxy UGC12591

Abstract

We present our XMM-Newton observation of the fastest rotating spiral galaxy UGC12591. We detect hot gas halo emission out to 80kpc from the galaxy center, and constrain the halo gas mass to be smaller than 4.5 × 1011 M ⊙. We also measure the temperature of the hot gas as T = 0.64 ± 0.03keV. Combining our x-ray constraints and the near-infrared and radio measurements in the literature, we find a baryon mass fraction of 0.03-0.05 in UGC12591, suggesting a missing baryon mass of 70% compared with the cosmological mean value. Combined with another recent measurement in NGC1961, the result strongly argues that the majority of missing baryons in spiral galaxies do not reside in their hot halos. We also find that UGC12591 lies significantly below the baryonic Tully-Fisher relationship. Finally, we find that the baryon fractions of massive spiral galaxies are similar to those of galaxy groups with similar masses, indicating that the baryon loss is ultimately controlled by the gravitational potential well. The cooling radius of this gas halo is small, similar to NGC1961, which argues that the majority of the stellar mass of this galaxy is not assembled as a result of cooling of this gas halo. © 2012. The American Astronomical Society. All rights reserved.