IUE observations of star formation in a cooling flow

Lene Hansen, H.E. Jørgensen, Hans Ulrik Nørgaard-Nielsen

Research output: Contribution to journalJournal articleResearchpeer-review

Abstract

Star formation in cooling flows is usually found to have an initial mass function deficient in massive stars, but the center of the cooling flow in Hydra A has been shown to contain a significant number of early type stars. Here we use UV-spectra obtained with the IUE satellite together with ground based data to constrain the nature of this young population. The data is compatible with a burst of star formation with a Salpeter-like initial mass function, a burst age of about 410(7) yr, and a total mass approximate to 10(8) M..
Original languageEnglish
JournalAstrophysics and Space Science
Volume257
Issue number2
Pages (from-to)311-318
ISSN0004-640X
Publication statusPublished - 1998

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