Chandra Spectroscopy and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages, 2 figures. Submitted to the proceedings of the 8th IAU Asian-Pasific Regional Meeting Volume 1

Scientific paper

We present the X-ray analysis and the mass estimation of the lensing cluster of galaxies CL0024+17 with Chandra. We found that the temperature profile is consistent with being isothermal and the average X-ray temperature is 4.47 (+0.83, -0.54) keV. The X-ray surface brightness profile is represented by the sum of emissions associated with the central three bright elliptical galaxies and the emission from intracluster medium (ICM) which can be well described by a spherical beta-model. Assuming the ICM to be in the hydrostatic equilibrium, we estimated the X-ray mass and found it is significantly smaller than the strong lensing mass by a factor of 3.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Chandra Spectroscopy and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17 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 Chandra Spectroscopy and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Spectroscopy and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-591427

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.