Chandra monitoring observation of the Antennae galaxies: the X-ray source populations and the shape of their luminosity function

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4

Galaxies: Antennae (Ngc 4038/39), X-Rays: Binaries, X-Rays: Galaxies

Scientific paper

We present the X-ray luminosity function (XLF) of the Antennae galaxies based on 8 observation performed with Chandra. We detect between 37 and 49 sources in each observation. After combining all observations we detect a total of 120 sources down to a limiting luminosity of ˜ 2x1037 erg s-1. Comparison between the XLFs of the individual observations shows that they are not affected by source variability. The cumulative XLF of the coadded observations is well represented by a single power-law with a slope of ˜ - 0.5.

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 monitoring observation of the Antennae galaxies: the X-ray source populations and the shape of their luminosity function 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 monitoring observation of the Antennae galaxies: the X-ray source populations and the shape of their luminosity function, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra monitoring observation of the Antennae galaxies: the X-ray source populations and the shape of their luminosity function will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-771779

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