Direct observations of bipolar outflow from HM sagittae

S. P S Eyres*, R. J. Cohen, R. J. Davis, H. T. Kenny, H. M. Lloyd, M. F. Bode, S. M. Dougherty

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

1 Citation (Scopus)


We observed HM Sagittae with the Multi-Element Radio Linked Interferometer Network (MERLIN) at 6 cm and 18cm. We find non-thermal bipolar outflow in the eastwest direction, associated with optical emission lines, and thermal ridges to the north and south associated with the UV nebulosity detected by the HST.

Original languageEnglish
Pages (from-to)457-458
Number of pages2
JournalAstrophysics and Space Science
Issue number1-2
Publication statusPublished - Feb 1995


  • binaries: symbiotic
  • radio continuum: stars
  • stars: individual: HM Sge


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