Deciphering the Universe through SpectroscopyRegina von Berlepsch This 22nd volume in the series contains 15 invited reviews and highlight contributions from outstanding speakers presented during the 2009 annual meeting of the Astronomical Society on the subject of "Deciphering the Universe through Spectroscopy", held in Potsdam, Germany. Topics range from the measurements of magnetic fields on the surface of the sun via detailed measurements of abundances in stellar atmospheres to the kinematics of the universe at its largest scales. The result is a systematic overview of the latest astronomical and cosmological research. |
Contents
1993 | |
1997 | |
1998 | |
1999 | |
2000 | |
2001 | |
References | |
Probing dark matter galaxies and the expansion history of the Universe | |
The EXOTIME program 6 Substellar companions of evolved stars 7 Summary | |
Xray spectroscopy and mass analysis of galaxy clusters 1 Xray observations of galaxy clusters | |
Mass models from Xray data | |
Testing cold dark matter | |
Cosmology with gas mass fractions of galaxy clusters | |
Outlook | |
The metallicities of galaxies | |
luminosity relationship FGLR | |
First distances using the FGLRmethod | |
The potential of FGLRmethod for extragalactic distance determinations | |
Perspectives of future work | |
The asteroseismologyextrasolarplanet connection 1 Introduction | |
Extrasolar planet detection methods | |
Stellar oscillation extrasolar planet links | |
Hot subdwarf stars | |
Ludwig Biermann Award Lecture | |
References | |
Quantitative solar spectroscopy | |
References | |
Acknowledgements | |
Acknowledgements References | |
Highfidelity spectroscopy at the highest resolutions 1 Why the highest resolution? | |
Solar and stellar spectra 3 Advancing highresolution spectroscopy | |
Intergalactic wavelength shifts in quasars | |
Spectrometers at the largest telescopes | |
Acknowledgements References | |
Spectroscopy of Solar Neutrinos 1 Introduction | |
The solar neutrino spectrum | |
Past and present experiments | |
The Borexino experiment | |
Solar neutrinos and solar metallicity | |
Potential of future experiments | |
Conclusions | |
General Index of Contributors | |
Common terms and phrases
absorption accretion rate Aoki asteroseismology Astronomy baryons Baumgardt Beers Belokurov binary black hole calibration chemical Christlieb Coma cosmic cosmological Curdt Daddi dark matter densities dark matter halos detection detector distribution dSph dwarf galaxies dynamical early-type ejection elemental abundances ellipticals emission energy evolution Fe/H Figure flux Frebel Galactic centre Galactic halo galaxy clusters galaxy formation gas mass Gilmore Haehnelt high redshift high-resolution hypervelocity stars IMBH irradiance kinematics Löckmann low-mass luminosity massive measurements mergers metal-poor metal-poor stars metallicity Milky MNRAS models molecular gas Norris observed optical orbital parameters photometry Phys planets population Portegies Portegies Zwart quasars r-process radiation range ratio Rauch redshift resolution S-stars sample satellite Schwarzschild shown in Fig simulations SMBH Sneden solar neutrino spatial spectral spectrometers spectroscopy spectrum spirals star formation star forming stellar mass subdwarf supergiants supernova telescopes temperature thick disk transition disk velocity wavelength Wilhelm Wyse X-ray