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

Published online by Cambridge University Press:  01 August 2006

M. Das
Affiliation:
Raman Research Institute, Bangalore 560 080, India; email: mousumi@rri.res.in
K. O'Neil
Affiliation:
NRAO, P.O. Box 2, Green Bank, WV 24944
N. Kantharia
Affiliation:
NCRA, TIFR, Post Bag 3, Ganeshkhind, Pune-411007, India
S. N. Vogel
Affiliation:
University of Maryland, College Park, MD 20742
S. S. McGaugh
Affiliation:
University of Maryland, College Park, MD 20742
Corresponding
E-mail address:
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Abstract

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Das, M., O'Neil, K., Vogel, S.N., & McGaugh, S.S. 2006, ApJ Oct 20, in press.Google Scholar
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