Starburst Galaxies as Recently Formed Companions

Abstract

Direct photography and spectra of the companion galaxy NGC 2777 show that it is composed predominantly of young stars and that it exhibits outflow of hot gaseous material. A hydrogen filament leads back to a larger nearby galaxy. it is proposed that this smaller, currently star forming companion, originated recently from material ejected from the larger galaxy.

Keywords

Dust Emissivity Photography 

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Copyright information

© Springer-Verlag Berlin Heidelberg 1988

Authors and Affiliations

  • H. Arp
    • 1
  1. 1.Institut für AstrophysikMax-Planck-Institut für Physik und AstrophysikGarchingFed.Rep.of Germany

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