Mapping the z=0.19 HI absorption against PKS1830-211

Physics – Optics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

The HI absorption feature in PKS1830-211 at z=0.19 is observed with the VLA in conjunction with the VLBA antenna at Pie Town (PT). The PT antenna was linked in real time to the VLA correlator through a new experimental state-of-the-art fiber optics link while the observations at 1191MHz accessed the lowest frequencies available in the 20cm band. The VLA-PT baselines allowed us to separate the two bright radio images in the Einstein ring at 1191 MHz, spatially resolving the HI absorption feature. We find similar absorption profiles against the two components, separated by 42 km/s. Each profile has an optical depth of 0.02 which corresponds to an HI column density of 1.2x1020 atoms/cm2 for a spin temperature of 100K. Deconvolved velocity dispersions are 12 km/s for the NE and 7 km/s for the SW component. These properties are typical for a normal galactic HI disk. Besides a red galaxy near the center of the Einstein ring, a recent HST-NICMOS image by Lehár et al (1999) also shows a bluer galaxy (G2) at 6.2 kpc to the south (H0=75 km/s/Mpc, q0=0.5, z=0.19). We identify G2 as the z=0.19 absorber since two other candidate galaxies in the HST image have impact parameters of 32 and 38 kpc at z=0.19. The NIR morphology of G2 suggests a near face-on late type galaxy which implies that the 42 km/s velocity difference hints at a rather massive system.

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

Mapping the z=0.19 HI absorption against PKS1830-211 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 Mapping the z=0.19 HI absorption against PKS1830-211, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mapping the z=0.19 HI absorption against PKS1830-211 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1740359

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