The gravitational lens hypothesis for 0846 + 51W1 supported by new observations

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16

Bl Lacertae Objects, Faint Objects, Gravitational Lenses, Red Shift, Astronomical Photometry, Elliptical Galaxies, Image Analysis, Spectrum Analysis, Visible Spectrum

Scientific paper

On deep direct images taken during a faint state, the high redshift BL Lac object 0846 + 51W1 shows an elongated appearance which is due to an intervening galaxy located nearly exactly on the line of sight. The optical emission of this galaxy is also present in the spectrum of 0846 + 51W1 and causes the apparently steep optical spectral index during the low quasar-like state of this object. Modeling the observed spectrum of 0846 + 51W1 with a quasar power law of spectral index alpha = 1.1 and the energy distribution of an elliptical galaxy yields a redshift of z = 0.235 for the intervening galaxy. These observations strongly support the hypothesis that the observed properties of 0846 + 51W1 are markedly influenced by gravitational (micro)lensing.

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

The gravitational lens hypothesis for 0846 + 51W1 supported by new observations 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 The gravitational lens hypothesis for 0846 + 51W1 supported by new observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The gravitational lens hypothesis for 0846 + 51W1 supported by new observations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1527266

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