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Water masers associated with compact molecular clouds and ultracompact Hii regions: The extended sample

  • R. Cesaroni
  • G. Comoretto
  • M. Felli
  • F. Palla
  • J. Brand
  • P. Caselli
7. Water Masers in Star-Forming Regions
Part of the Lecture Notes in Physics book series (LNP, volume 412)

Abstract

We present the results of a survey of water maser emission at 22.2 GHz towards a selected sample of IRAS-PSC sources which are believed to be associated with very young massive stars. The sample consists of 591 sources. The observations have been carried out using the Medicina 32-m radiotelescope, operated by the Istituto di Radioastronomia - C.N.R., Bologna.

Whereas previous searches for maser emission have been directed towards known Hii regions, the aim of the present survey is to identify new sources in an even earlier evolutionary phase, corresponding to the development of an ultracompact Hii region. It is shown that our sample contains a significant number of sources that could be considered good candidates of massive protostellar cores still in the main accretion phase.

Keywords

Color Index Early Evolutionary Phase Intermediate Mass Star Color Criterion Young Massive Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Springer-Verlag 1993

Authors and Affiliations

  • R. Cesaroni
    • 1
  • G. Comoretto
    • 1
  • M. Felli
    • 1
  • F. Palla
    • 1
  • J. Brand
    • 2
  • P. Caselli
    • 2
  1. 1.Osservatorio Astrofisico di ArcetriFirenzeItaly
  2. 2.Istituto di RadioastronomiaBolognaItaly

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