Abstract
The starburst plus radio hypernovae scenario presented for high-luminosity (HLIRGs) and ultraluminous IRAS galaxies (ULIRGs) in Colina & Perez-Olea (1992) is used to predict the [Fe II] 1.64 μm luminosity in these galaxies, as well as the [Fe II] 1.64 μm, radio, and Brγ luminosity rates. These are good indicators to characterize starbursts in heavily obscured environments, i.e., buried starbursts, such as those believed to exist in HLIRGs and ULIRGs. The predicted [Fe II] 1.64 μm luminosity for HLIRGs and ULIRGs is in the range 10 40 -10 42 ergs s −1 while the rate of [Fe II] 1.64 μm to radio luminosity, with a mean value of 17, is almost independent of the initial mass function parameters
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
