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 |
|---|---|
| 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