NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-06-16 T22:53:25 PDT
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For refcode 2000A&A...355..922J:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
2000A&A...355..922J The FIR-radio correlation of Wolf-Rayet galaxies and the role of star formation in LINERs. JI L., CHEN Y., HUANG J.H., GU Q.S., LEI S.J. Received 14 October 1999/Accepted 20 January 2000 Abstract: We find that a preliminary classification of LINERs' energetics may be made in terms of the FIR-radio correlation of Wolf-Rayet galaxies. The AGN- or starburst-supported LINERs can be distinguished by their FIR- to-radio ratio, Q=L(1.4GHz)/L(60microns) > or < 0.01. It is interesting to note that almost all the LINERs with inner rings might be starburst- supported, indicating reduced AGN activities compared with those of the AGN-supported ones. We also find that a shock-heating phase for the warm dust component might be important for some starbursts at the burst age of >=10^7^yr, with Q<0.001. Key words: galaxies: active - infrared: galaxies - radio continuum: galaxies
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