The outflows from the symbiotic nebulae He 2--147 and HM SGE
Symbiotic stars, which are interacting binary stars usually composed by a late type giant and a very hot/luminous white dwarf, are a powerful laboratory to investigate mass loss phenomenon relevant to a wide range of astrophysical topics: aspherical mass loss, collimated winds from accretion disks, colliding winds, mass loss induced by violent
Brandi, E. et al.
Fecha de publicación:
11
1998