Possible pulsations of the M giant in MWC560
| dc.creator | Frackowiak, Sylwia M. | |
| dc.creator | Mikolajewski, Maciej | |
| dc.creator | Tomov, Toma | |
| dc.date | 2002-10-19 | |
| dc.date.accessioned | 2026-07-07T02:05:47Z | |
| dc.date.available | 2026-07-07T02:05:47Z | |
| dc.description | MWC 560 and other peculiar symbiotic binary, CH Cyg, have been classified as the prototypes of the new subclass of symbiotic systems - propellers, with accretion onto a magnetic white dwarf being the source of activity. The companion of the hot component in this model should demonstrate stellar wind with relatively high mass-loss. It can be expected rather a late AGB, Mira or semiregular variable (SR) than any normal red giant.Our analysis performed for the I band shows that the M giant probably belongs to such kind of stars and pulsates with a period of about 5 months. | |
| dc.description | 4 pages, 2 figures, to appear in the proceedings of "Symbiotic stars probing stellar evolution", R.L.M.Corradi, J.Mikolajewska, T.J.Mahoney eds., 2002, ASP Conference Series, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0210447 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0210447 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5206 | |
| dc.subject | Astrophysics | |
| dc.title | Possible pulsations of the M giant in MWC560 | |
| dc.type | text |