Thomas Bensby
Senior lecturer
THE Gaia-ESO Survey : Metal-rich bananas in the bulge
Author
Summary, in English
We analyze the kinematics of ∼2000 giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region -10° ≲ l≲ 10° and -11° ≲ b ≲ -3°. We find distinct kinematic trends in the metal-rich ([M H] > 0) and metal-poor ([M H] <0) stars in the data. The velocity dispersion of the metal-rich stars drops steeply with latitude, compared to a flat profile in the metal-poor stars, as has been seen previously. We argue that the metal-rich stars in this region are mostly on orbits that support the boxy-peanut shape of the bulge, which naturally explains the drop in their velocity dispersion profile with latitude. The metal-rich stars also exhibit peaky features in their line of sight velocity histograms, particularly along the minor axis of the bulge. We propose that these features are due to stars on resonant orbits supporting the boxy-peanut bulge. This conjecture is strengthened through the comparison of the minor axis data with the velocity histograms of resonant orbits generated in simulations of buckled bars. The "banana" or 2:1:2 orbits provide strongly bimodal histograms with narrow velocity peaks that resemble the Gaia-ESO metal-rich data.
Department/s
- Lund Observatory - Has been reorganised
- Department of Astronomy and Theoretical Physics - Has been reorganised
Publishing year
2016-06-20
Language
English
Publication/Series
Astrophysical Journal Letters
Volume
824
Issue
2
Document type
Journal article
Publisher
IOP Publishing
Topic
- Astronomy, Astrophysics and Cosmology
Keywords
- galaxies: general
- galaxies: kinematics and dynamics
- Galaxy: bulge
Status
Published
Project
- Gaia-ESO Survey
ISBN/ISSN/Other
- ISSN: 2041-8205