Artikel
Open Access
The velocity field and 3-D structure of the Universe
-
E. Høg
Veröffentlicht/Copyright:
16. März 2017
Published Online: 2017-3-16
Published in Print: 1999-6-1
© 2017
Artikel in diesem Heft
- Contents
- Proceedings of the Gaia Workshop
- Gaia: the galactic central bulge
- Predicting Gaia observations from a star-count model
- Luminosity calibration and distance scale
- The Cepheid-Based Distance Scale
- The Spatial Resolution of the Extinction Structure from Gaia
- The star formation history of the Milky Way: methodology and implications for Gaia
- The velocity field and 3-D structure of the Universe
- Prospects for astrometric measurements of gravitational waves from stellar sources with Gaia
- Gaia and the evolution of young stars
- Testing stellar structure and evolution with Gaia
- Unraveling the history of star formation in the galactic disk with Gaia
- A few remarks on AGB variable stars and the Gaia mission
- Gaia science output: white dwarfs
- On derivation of masses of the SB2 components with Gaia astrometry
- The impact of high accuracy astrometry on asteroseismology
- First thoughts about variable star analysis
Creative Commons
BY-NC-ND 4.0
Artikel in diesem Heft
- Contents
- Proceedings of the Gaia Workshop
- Gaia: the galactic central bulge
- Predicting Gaia observations from a star-count model
- Luminosity calibration and distance scale
- The Cepheid-Based Distance Scale
- The Spatial Resolution of the Extinction Structure from Gaia
- The star formation history of the Milky Way: methodology and implications for Gaia
- The velocity field and 3-D structure of the Universe
- Prospects for astrometric measurements of gravitational waves from stellar sources with Gaia
- Gaia and the evolution of young stars
- Testing stellar structure and evolution with Gaia
- Unraveling the history of star formation in the galactic disk with Gaia
- A few remarks on AGB variable stars and the Gaia mission
- Gaia science output: white dwarfs
- On derivation of masses of the SB2 components with Gaia astrometry
- The impact of high accuracy astrometry on asteroseismology
- First thoughts about variable star analysis