Jet-Induced Star Formation
نویسندگان
چکیده
منابع مشابه
Anomalous H I kinematics in Centaurus A : evidence for jet - induced star formation
We present new 21-cm H I observations performed with ATCA of the large H I filament located about 15 kpc NE from the centre of Centaurus A and discovered by Schiminovich et al. (1994). This H I cloud is situated (in projection) near the radio jet of Centaurus A, as well as near a large filament of ionised gas of high excitation and turbulent velocities and near regions with young stars. The hig...
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The high redshift radio galaxy 4C41.17 has been shown in earlier work to consist of a powerful radio source in which there is strong evidence for jet-induced star formation along the radio axis. We argue that nuclear photoionization is not responsible for the excitation of the emission line clouds and we construct a jet-cloud interaction model to explain the major features revealed by the detai...
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Starbursts produce large numbers of Young Star Clusters (YSCs). Multi-color photometry in combination with a dedicated SED analysis tool allows to derive ages, metallicities, EB−V, and masses including 1σ uncertainties for individual clusters and, hence, mass functions for YSC systems. The mass function, known to be Gaussian for old Globular Cluster (GC) systems, is still controversial for YSC ...
متن کاملJet - Induced Emission - Line Nebulosity and Star Formation in the High - Redshift Radio Galaxy 4 C 41 . 17 Geoffrey
The high redshift radio galaxy 4C41.17 has been shown in earlier work to consist of a powerful radio source in which there is strong evidence for jet-induced star formation along the radio axis. We argue that nuclear photoionization is not responsible for the excitation of the emission line clouds along the axis of the radio source and we therefore construct a jet-cloud interaction model to exp...
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Analyzing global starburst properties in various kinds of starburst and post-starburst galaxies and relating them to the properties of the star cluster populations they form, I explore the conditions for the formation of massive, compact, long-lived star clusters. The aim is to find out whether the relative amount of star formation that goes into star cluster formation as opposed to field star ...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 2004
ISSN: 0074-1809
DOI: 10.1017/s0074180900198225