activity
19972008
most citedalpha-, r-, and s-process element trends in the Galactic thin and thick disks

631 citations · 1.3k across the 14 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph2006134 cited

Disentangling the Hercules stream

T. Bensby, M. S. Oey, S. Feltzing +1

Using high-resolution spectra of nearby F and G dwarf stars, we have investigated the detailed abundance and age structure of the Hercules stream. We find that the stars in the str…

astro-ph2006

Hercules stream stars and the metal-rich thick disk

T. Bensby, M. S. Oey, S. Feltzing +1

Using the MIKE spectrograph, mounted on the 6.5 m Magellan/Clay telescope at the Las Campanas observatory in Chile, we have obtained high-resolution spectra for 60 F and G dwarf st…

astro-ph200641 cited

Absolute diffuse calibration of IRAC through mid-infrared and radio study of HII regions

Martin Cohen, Anne J. Green, Marilyn R. Meade +9

We investigate the diffuse absolute calibration of the InfraRed Array Camera on the Spitzer Space Telescope at 8.0microns using a sample of 43 HII regions with a wide range of morp…

astro-ph200656 cited

Technetium and the third dredge up in AGB stars II. Bulge stars

Stefan Uttenthaler, Josef Hron, Thomas Lebzelter +3

We searched for Technetium (Tc) in a sample of bright oxygen-rich asymptotic giant branch (AGB) stars located in the outer galactic bulge. Tc is an unstable element synthesised via…

astro-ph20067 cited

3D Studies of Neutral and Ionised Gas and Stars in Seyfert and Inactive Galaxies

C. G. Mundell, G. Dumas, E. Schinnerer +8

We are conducting the first systematic 3D spectroscopic imaging survey to quantify the properties of the atomic gas (HI) in a distance-limited sample of 28 Seyfert galaxies and a s…

astro-ph2006207 cited

Simulating Cosmic Reionization at Large Scales II: the 21-cm Emission Features and Statistical Signals

Garrelt Mellema, Ilian T. Iliev, Ue-Li Pen +1

We present detailed predictions for the redshifted 21cm signal from the epoch of reionization. These predictions are obtained from radiative transfer calculations on the results of…