Groups and the Entropy Floor- XMM-Newton Observations of Four Groups

Details Groups and the Entropy Floor- XMM-Newton Observations of Four Groups Groups and the Entropy Floor- XMM-Newton Observations of Four Groups

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.1307f&link_type=abstract

American Astronomical Society, HEAD meeting #7, #13.07; Bulletin of the American Astronomical Society, Vol. 35, p.618

Other

Scientific paper

Using XMM-Newton spatially resolved X-ray imaging spectroscopy we obtain the temperature, density, entropy, gas mass, and total mass profiles for four groups of galaxies (NGC4325, NGC2563, NGC2300, and NGC5129) out to ˜0.3Rvir (Rvir, the virial radius). Our density profiles agree well with those derived previously, and the temperature data are broadly consistent with previous results but are considerably more precise. These groups are at the mass scale of 2x1013 Msolar but have rather different properties. They have considerably lower gas mass fractions at r<0.3Rvir than the rich clusters. NGC2563, one of the least luminous groups for its X-ray temperature, has a very low gas mass fraction of ˜0.004 inside 0.1 Rvir, which rises with radius. NGC4325, one of the most luminous groups at the same average temperature, has a higher gas mass fraction of 0.02. The entropy profiles and the absolute values of the entropy as a function of virial radius also differ, with NGC4325 having a value of ˜100 keV cm-2 and NGC2563 a value of ˜300 keV cm-2 at r ˜0.1 Rvir, and the other groups in between. The profiles rise monotonically with radius and there is no sign of an entropy floor. These results are inconsistent with pre-heating scenarios which have been developed to explain the entropy floor in groups but are broadly consistent with models of structure formation which include the effects of heating and/or the cooling of the gas. The total entropy in these systems provides a strong constraint on all models of galaxy and group formation, and on the poorly defined feedback process which controls the transformation of gas into stars and thus the formation of structure in the universe.

Affiliated with

Also associated with

No associations

Rating

Groups and the Entropy Floor- XMM-Newton Observations of Four Groups does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Groups and the Entropy Floor- XMM-Newton Observations of Four Groups, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Groups and the Entropy Floor- XMM-Newton Observations of Four Groups will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-999125