The Galactic Stellar Disc
arXiv:0811.1777 · doi:10.1088/0031-8949/2008/T133/014031
Abstract
The study of the Milky Way stellar discs in the context of galaxy formation is discussed. In particular we explore the properties of the Milky Way disc using a new sample of about 550 dwarf stars for which we have recently obtained elemental abundances and ages based on high resolution spectroscopy. For all the stars we also have full kinematic information as well as information about their stellar orbits. We confirm results from previous studies that the thin and the thick disc have distinct abundance patterns. But we also explore a larger range of orbital parameters than what has been possible in our previous studies. Several new results are presented. We find that stars that reaches high above the galactic plane and have eccentric orbits show remarkably tight abundance trends. This implies that these stars formed out of well mixed gas that had been homogenized over large volumes. We find some evidence that point to that the event that most likely caused the heating of this stellar population happened a few billion years ago. Through a simple, kinematic exploration of stars with super-solar [Fe/H] we show that the solar neighbourhood contains metal-rich, high velocity stars that very likely are associated with the thick disc. Additionally, the HR1614 moving group and the Hercules and Arcturus stellar streams are discussed and it is concluded that, probably, a large fraction of the so far identified groups and streams in the disc are the result of evolution and interactions within the stellar disc rather than being dissolved stellar clusters or engulfed dwarf galaxies.
20 pages, Review talk at the conference "A stellar journey", A symposium in celebration of Bengt Gustafsson's 65th birthday, held in Uppsala, June 2008, In press in Physica Scripta, eds. Paul Barklem, Andreas Korn, and Bertrand Plez
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Cited by in corpus (19)
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- New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey
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- On the angular momentum evolution of fully-convective stars: rotation periods for field M-dwarfs from the MEarth transit survey
- A rocky planet transiting a nearby low-mass star
- Characterizing the Cool KOIs III. KOI-961: A Small Star with Large Proper Motion and Three Small Planets
- Verifying asteroseismically determined parameters of Kepler stars using hipparcos parallaxes: self-consistent stellar properties and distances
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- Towards stellar effective temperatures and diameters at one per cent accuracy for future surveys
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- Observational Evidence from SDSS for a Merger Origin of the Milky Way's Thick Disk
- High- and Low- Disk Stars Separate Dynamically at all Ages
- Photometric rotation periods for 107 M dwarfs from the APACHE survey
- Deceleration of kicked objects due to the Galactic potential
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- The Spheroidal Bulge of the Milky Way: Chemodynamically Distinct from the Inner-Thick Disc and Bar