Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies

Details Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies

2006-09-15

arxiv.org/abs/astro-ph/0609426v1

Astronomy and Astrophysics

Astrophysics

one page; submitted to proceedings of IAU Symposium 235: Galaxy Evolution across the Hubble Time

Scientific paper

LSB galaxies have low metallicities, diffuse stellar disks, and massive HI disks. We have detected molecular gas in two giant LSB galaxies, UGC 6614 and F568-6. A millimeter continuum source has been detected in UGC 6614 as well. At centimeter wavelengths we have detected and mapped the continuum emission from the giant LSB galaxy 1300+0144. The emission is extended about the nucleus and is most likely originating from the AGN in the galaxy. The HI gas distribution and velocity field in 1300+0144 was also mapped. The HI disk extends well beyond the optical disk and appears lopsided in the intensity maps.

Affiliated with

Also associated with

No associations

Rating

Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies 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 Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Observations of the AGN and Gas in Low Surface Brightness Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-409714