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- W90403603 abstract "This paper has studied the correlation between luminosity of 66 OH mega-masers and infrared luminosity of their host galaxies. A relation log L(OH)=1.71 log L(IR)-17.67, i.e. L(OH) [L(IR)]1.71, is obtained. The resultis interposed between L(OH) [L(IR)]2 obtained by Baan(1989)and L(OH) oc [L(IR)]1.38 obtained by Kandalian(1996). Because the sample number is the largest among the mentioned results,our result closes the practical condition. Furthermore, the 66 OH megamasers can be divided in two groups. First group is the OH megamasers having small luminosity of L(OH)102L, which contains 14 OH megamasers. Second one is one having large luminosity of L(OH)102L, which contains 52 OH megamasers. Our results indicate, the correlation between luminosity of OH megamasers having small luminosity and infrared luminosity of their host galaxies is L(OH) oc [L(IR)]1.43, which closes one obtained by Kandalia(1996), and the correlation between luminosity of OH megamaser having large luminosity and infrared luminosity of their host galaxies is L(OH) [L(IR)]2 , which is the same one obtained by Baan(1989)." @default.
- W90403603 created "2016-06-24" @default.
- W90403603 creator A5048375787 @default.
- W90403603 date "2002-01-01" @default.
- W90403603 modified "2023-09-24" @default.
- W90403603 title "Correlation between Luminosity of OH Megamasers and Infrared Luminosity of Their Host Galaxies" @default.
- W90403603 hasPublicationYear "2002" @default.
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