OH Megamaser Galaxies at High Angular Resolution

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

Here we discuss the results of VLBI observations of OH megamasers in ultra-luminous infrared galaxies. To date, in all OH megamaser sources observed with VLBI a large part of the OH maser emission is associated with circumnuclear disks or tori. The most striking result is that of III Zw 35, where the maser emission appears to be in a ring-like structure. This ring geometry can explain the two compact clumps of emission previously observed, and theoretical modeling using a torus can successfully reproduce the observed emission. In some OH megamaser galaxies new data further suggests that in addition to an OH maser disk, some maser emission may also be associated with outflows.

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

OH Megamaser Galaxies at High Angular Resolution 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 OH Megamaser Galaxies at High Angular Resolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OH Megamaser Galaxies at High Angular Resolution will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1032692

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