Radio Continuum and CO emission in spiral galaxies
Date Issued
2004
Author(s)
•
•
Helfer, T.
•
Ekers, R.
•
Blitz, L.
•
•
Wong, T.
•
Gregorini, L.
Abstract
We have studied the relationship between the Radio Continuum (RC) and CO emission for a set of galaxies selected from the BIMA SONG sample. By combining new 20 cm VLA B-array observations with BIMA maps it has been possible to investigate the behaviour of the RC/CO correlation at matched resolution down to an angular size of about 6''. Preliminary results indicate that the RC/CO correlation is as tight as (if not better than) the famous RC/FIR one. This may have important consequences on the models proposed to explain them.
Coverage
48th Annual Meeting of the Italian Astronomical Society, I Colori dell'Universo
All editors
Wolter, A.; Israel, G. L.; Bacciotti, F.
Volume
5
Start page
280
Conferenece
48th Annual Meeting of the Italian Astronomical Society, I Colori dell'Universo
Conferenece place
Milano, Italy
Conferenece date
April 19-23, 2004
Issn Identifier
0037-8720
Ads BibCode
2004MSAIS...5..280P
Rights
open.access
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