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CO Outflows and H2O Masers: What Type of Connection?

  • M. Felli
  • F. Palagi
  • G. Tofani
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 186)

Abstract

In this contribution we discuss the relationship between the (616 → 523) H2O maser emission and the CO molecular outflows found in star forming regions, for a sample of 142 confirmed outflows.

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References

  1. Beichman, C.A., Neugebauer, G., Habing, H.J., Clegg, P.E., Chester, T.J.: 1984, IRAS Catalogs and Atlas Eplanatory Supplement Google Scholar
  2. Elitzur, M., Hollenbach, D.J., McKee, C.F.: 1989, Astrophys. J. 346, 983ADSCrossRefGoogle Scholar
  3. Felli, M., Palagi, F., Tofani, G.: 1991, Astron. Astrophys. 255, 293ADSGoogle Scholar
  4. Fukui, J.: 1989, in B. Reipurth, ed(s)., Low mass star formation and pre-main sequence objects,ESO workshop, 95Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  • M. Felli
    • 1
  • F. Palagi
    • 2
  • G. Tofani
    • 1
  1. 1.Osservatorio Astrofisico di ArcetriFirenzeItaly
  2. 2.Gruppo Nazionale Astronomia, U.d.R. ArcetriC.N.R.FirenzeItaly

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