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Chemical evolution of ytterbium in the Galactic disk*
Preliminary results of the 2001-2002 Gemini sodium monitoring campaign at Cerro Tololo, Chile
One year of Galileo dust data from the Jovian system: 1996
The dust detector system onboard Galileo has recoding dust impacts incircumjovian space since the spacecraft was injected into a bound orbitabout Jupiter in December 1995. This is the sixth in a series of papersdedicated to presenting Galileo and Ulysses dust data. We present datafrom the Galileo dust instrument for the period January to December 1996when the spacecraft completed four orbits about
Galileo observes electromagnetically coupled dust in the Jovian magnetosphere
Measurements of dust coupled to the Jovian magnetosphere have been obtained with the dust detector on board the Galileo spacecraft. We report on data obtained during the first four orbits about Jupiter that had flybys of the Galilean satellites: Ganymede (orbits 1 and 2), Callisto (orbit 3), and Europa (orbit 4). The most prominent features observed are highly time variable dust streams recorded t
Extended term analysis of Mo II
The Carlina-type diluted telescope Stellar fringes on Deneb
s-Process elements in the M supergiant alpha Ori
We present new results on a study of the weak s-process elemental abundances in the M supergiant alpha Ori (M2Iab). We have conducted the abundance analysis through comparison of synthetic with observed spectra in the two infrared spectral regions 0.7 - 1.1 mu m and 2.1 - 2.3 mu m, where the molecular and atomic line densities are less than in the optical region and where many of the relevant elem
Astronomical applications of quantum optics for extremely large telescopes
Chemical evolution of fluorine in the bulge High-resolution K-band spectra of giants in three fields
A portable high-resolution soft x-ray and extreme ultraviolet spectrometer designed for the Shanghai EBIT and the Shanghai low energy EBITs
The FERRUM project: metastable lifetimes in Cr II
Parity forbidden radiative transitions from metastable levels are observed in spectra of low-density astrophysical plasmas. These lines are used as probes of the physical conditions, made possible due to the long lifetime of their upper level. In a joint effort, the FERRUM project aims to obtain new and accurate atomic data for the iron-group elements, and part of this project concerns forbidden l
Implementing the Gaia Astrometric Global Iterative Solution (AGIS) in Java
On the numerical treatment and dependence of thermohaline mixing in red giants
Fluorine in the Solar Neighborhood: Is It All Produced in Asymptotic Giant Branch Stars?
On the origin of black hole spin in high-mass black hole binaries: Cygnus X-1
Prospects of stellar abundance studies from near-IR spectra observed with the E-ELT
All-sky search for periodic gravitational waves in the full S5 LIGO data
We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6 x 10(-9) Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10x increase in computational efficienc
The FERRUM Project: Experimental oscillator strengths of the UV 8 multiplet and other UV transitions from the y6P levels of Fe II
We report on experimental branching fractions (BFs) for 19 transitions from the three 3d 5( 6S)4s4p( 3P) y6P levels in Fe II, measured in Fourier transform spectra of a Penning discharge lamp and a hollow cathode lamp. The transition wavelengths span the interval between 1600 and 2850 Å. Absolute oscillator strengths ( f-values) have been derived by combining the BFs with experimental radiative li
Laser control of atoms and molecules
Rather different problems can be lumped together under the general term 'laser control of atoms and molecules'. They include the laser selection of atomic and molecular velocities for the purpose of Doppler-free spectroscopy, laser control of the position and velocity of atoms (i.e. laser trapping and cooling of atoms), and laser control of atomic and molecular processes (ionization, dissociation)
