Abstract
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 language | English |
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Pages (from-to) | 457-458 |
Number of pages | 2 |
Journal | Astrophysics and Space Science |
Volume | 224 |
Issue number | 1-2 |
DOIs | |
Publication status | Published - Feb 1995 |
Keywords
- binaries: symbiotic
- radio continuum: stars
- stars: individual: HM Sge