Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541202q&link_type=abstract
American Astronomical Society, AAS Meeting #215, #412.02; Bulletin of the American Astronomical Society, Vol. 42, p.246
Astronomy and Astrophysics
Astronomy
Scientific paper
In 2007, the pre-biotic molecule, methanimine (CH2NH), was detected in the Arecibo single-dish radio line spectrum of Arp 220. At a distance of 77 Mpc (z=0.018126), Arp 220 is the nearest Ultra-Luminous Infra-Red Galaxy (ULIRG), its IR luminosity arising from a powerful, dust-enshrouded starburst, triggered by the merger of two counter-rotating gas-rich galaxies. Evidence for this is provided by high resolution optical and radio images, revealing a double-nucleus structure with tidal tails, dust lanes and a large number of radio supernovae. Arp 220 is also the prototype OH megamaser galaxy, with VLBI maps of the 1665/1667 MHz transitions revealing complex emission regions. The object of our present study is to determine where in this complicated structure the site of the CH2NH molecules is located. To this end, we have acquired and imaged MERLIN observations of this line in Arp 220 at 40 mas resolution. We present both the results and our conclusions drawn from these in this poster.
Ghosh Tamal
Minchin Robert
Qasim Danna
Salter Chris
Thomasson Peter
No associations
LandOfFree
Merlin Imaging Of Methanimine Molecule (CH2NH) In Arp 220 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 Merlin Imaging Of Methanimine Molecule (CH2NH) In Arp 220, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Merlin Imaging Of Methanimine Molecule (CH2NH) In Arp 220 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-965746