Observations of the Optical Jet of MH 2136-428

Details Observations of the Optical Jet of MH 2136-428 Observations of the Optical Jet of MH 2136-428

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1057p&link_type=abstract

Chandra Proposal ID #04700004

Physics

Chandra Proposal Id #04700004

Scientific paper

We will image MH 2136-428 with HST/ACS in three bands: F475W, F625W, F850LP, i.e., SDSS g, r, z. The Chandra exposure time has been determined based on the results of Pesce et al. (2001) on 3C 371. The optical jet of this source has a surface brightness roughly 1.5 magnitudes fainter than that of our source, but the S/N ratio of the Chandra observations was far from optimal. Assuming that the X-ray-to-optical ratio of the jet in MH 2136-428 is similar to that of 3C 371, 10ks should allow us to constrain the presence of an X-ray jet without reasonable doubt.

Affiliated with

Also associated with

No associations

Rating

Observations of the Optical Jet of MH 2136-428 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 Observations of the Optical Jet of MH 2136-428, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of the Optical Jet of MH 2136-428 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1312923