The FIR-Radio Correlation of Wolf-Rayet Galaxies and the Role of Star Formation in LINERs

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dc.creatorJi, L.
dc.creatorChen, Y.
dc.creatorHuang, J. H.
dc.creatorGu, Q. S.
dc.creatorLei, S. J.
dc.date2000-01-26
dc.date.accessioned2026-07-07T06:28:06Z
dc.date.available2026-07-07T06:28:06Z
dc.descriptionWe 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, $Q\equiv L(1.4{\rm GHz})/$ $L(60μ{\rm m})>$ 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 $\ge 10^{7}$ yr, with $Q<0.001$.
dc.description9 pages, 4 figures, to be published in Astronomy & Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/0001445
dc.identifierhttp://arxiv.org/abs/astro-ph/0001445
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97619
dc.subjectAstrophysics
dc.titleThe FIR-Radio Correlation of Wolf-Rayet Galaxies and the Role of Star Formation in LINERs
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