|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Canis Major overdensity and Monoceros ring explained in terms of pure Milky Way structure
If you have a question about this talk, please contact Sergey Koposov.
Some authors have suggested the existence of a nearby dwarf galaxy associated to the Canis Major overdensity, which was tidally disrupted leaving remnants throughout the Monoceros ring observed along several positions within ~20 degrees from the Galactic plane. Here, we present arguments to think that the Canis Major overdensity is just a part of the Galactic warp+flare, instead of a dwarf galaxy or a new substructure in the Galaxy, and the Monoceros ring overdensities and its features on color-magnitude diagrams are mainly populations of the most external non-truncated flared thin+thick stellar disc. Failures to fit these features with the Milky structure stem mainly from the use of Galactic models which do not represent appropriately the southern warp, the disc flare, and that set an unrealistic truncation of the stellar populations of the disc at R>=14 kpc, like the Besançon model.
This talk is part of the Institute of Astronomy Galaxies Discussion Group series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsCIMR Professional Development Seminars Inorganic Chemistry Graduate and internship applications
Other talksDeath and sanitation: Imperial representations of The Ganges Does Photography Capture a Moment in Time? Divisor braids and gauge theory The Conscious Phenotype Caveolae protect endothelial cells from rupture during increased cardiac output The Cambridge Cognitive Neuroscience Research Panel