Accretion disks in Algols: progenitors and evolution

There are only a few Algols with measured accretion disk parameters. These measurements provide additional constraints for tracing the origin of individual systems, narrowing down the initial parameter space. We investigate the origin and evolution of 6 Algol systems with accretion disks to find the initial parameters and evolutionary constraints for them. With a modified binary evolution code, series of close binary evolution are calculated to obtain the best match for observed individual systems. Initial parameters for 6 Algol systems with accretion disks were determined matching both the present system parameters and the observed disk characteristics. When RLOF starts during core hydrogen burning of the donor, the disk lifetime was found to be short. The disk luminosity is comparable to the luminosity of the gainer during a large fraction of the disk lifetime.Comment: 8 pages, 6 figures , accepted by A&

Raman anemometry, a method for component-selective velocity measurements of particles in a flow

An anemometer for the measurement of the velocity of particles of different substances in a flow, separate and apart from that of the flow itself, is described. The substances are distinguished by Raman scattering. The velocity is obtained by relating the autocorrelated scattering signal to the known laser beam profile

A Raman spectroscopic study of the interaction between nucleotides and the DNA binding protein gp32 of bacteriophage T4

Raman spectra of the bacteriophage T4 denaturing protein gp32, its complex with the polynucleotides poly(rA), poly(dA), poly(dT), poly(rU), and poly(rC), and with the oligonucleotides (dA)8 and (dA)2, were recorded and interpreted. According to an analysis of the gp32 spectra with the reference intensity profiles of Alix and co-workers [M. Berjot, L. Marx, and A.J.P. Alix (1985) J. Ramanspectrosc., submitted; A.J.P. Alix, M. Berjot, and J. Marx (1985) in Spectroscopy of Biological Molecules, A. J. P. Alix, L. Bernard, and M. Manfait, Eds., pp. 149-154], 1 gp32 contains ≈ 45% helix, ≈ 40% β-sheet, and 15% undefined structure. Aggregation of gp32 at concentrations higher than 40 mg/mL leads to a coordination of the phenolic OH groups of 4-6 tyrosines and of all the sulfhydryl (SH) groups present in the protein with the COO- groups of protein. The latter coordination persists even at concentrations as low as 1 mg/mL. In polynucleotide-protein complexes the nucleotide shields the 4-6 tyrosine residues from coordination by the COO- groups even at high protein concentration. The presence of the nucleotide causes no shielding of the SH groups. With Raman difference spectroscopy it is shown that binding of the protein to a single-stranded nucleotide involves both tyrosine and trytophan residues. A change in the secondary structure of the protein upon binding is observed. In the complex, gp32 contains more -sheet structure than when uncomplexed. A comparison of the spectra of complexed poly(rA) and poly(dA) with the spectra of their solution conformations at 15°C reveals that in both polynucleotides the phosphodiester vibration changes upon complex formation in the same way as upon a transition from a regular to a more disordered conformation. Distortion of the phosphate-sugar-base conformation occurs upon complex formation, so that the spectra of poly(rA) and poly(dA) are more alike in the complex than they are in the free polynucleotides. The decrease in intensity of the Raman bands at 1304 cm-1 in poly(rA), at 1230 cm-1 in poly(rU), and at 1240 and 1378 cm-1 of poly(dT) may be indicative of increased stacking interactions in the complex. No influence of the nucleotide chain length upon the Raman spectrum of gp322 in the complex was detected. Both the nucleotide lines and the protein lines in the spectrum of a complex are identical in poly(dA) and (dA)8

The cytodisk: A cytometer based upon a new principle of cell alignment

A new method is described for one-dimensional alignment of small particles such as biological cells. A drop of the particle suspension is spread out on a flat disk or plate equipped with V-shaped grooves such as are present on a gramophone disk. After drying, the particles are located on the bottom of the grooves and are thus aligned in a one-dimensional array. The new alignment procedure is demonstrated with a suspension of fluorescent polystyrene micropheres (diameter 3.8 µm) and a suspension of the unicellular algae chlorella vulgaris (diameter about 3 µm). It appears that the alignment of cells and spheres is very good. \ud When using microspheres, more than 95% of the particles in the grooves are located within ±2 µm of the centre line of the groove. Based upon this cell-alignment principle, a new cytometer, named the cytodisk, is proposed. The proposed system has a number of advantages over the flow cytometer, among which is the unique ability of relocating a previously measured cell for further measurement or visual examination. \ud A prototype of a cytodisk, developed for initial test measurements, was built in our laboratory. The apparatus, constructed from a record player and ordinary long-playing records, uses a simple mechanical tracking system and a single optical fiber for fluorescence excitation and detection. With this apparatus it is demonstrated that a cytodisk can indeed perform quite well: A histogram of fluorescing microspheres could be measured with a coefficient of variation of 4.1%. The performance of this prototype is limited by the quality of the mechanical tracking system and the optical system used. It is expected that considerable improvements may be obtained by using a more sophisticated optical detection system such as the tracking system in use in optical disk players

The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters

Context. The chemical processes during the Asymptotic Giant Branch (AGB) evolution of intermediate mass single stars predict most of the observations of the different populations in globular clusters although some important issues still need to be further clarified. In particular, to reproduce the observed anticorrelations of Na-O and Al-Mg, chemically enriched gas lost during the AGB phase of intermediate mass single stars must be mixed with matter with a pristine chemical composition. The source of this matter is still a matter of debate. Furthermore, observations reveal that a significant fraction of the intermediate mass and massive stars are born as components of close binaries. Aims. We will investigate the effects of binaries on the chemical evolution of Globular Clusters and on the origin of matter with a pristine chemical composition that is needed for the single star AGB scenario to work Methods. We use a population synthesis code that accounts for binary physics in order to estimate the amount and the composition of the matter returned to the interstellar medium of a population of binaries. Results. We demonstrate in the present paper that the mass lost by a significant population of intermediate mass close binaries in combination with the single star AGB pollution scenario may help to explain the chemical properties of the different populations of stars in Globular Clusters.Comment: 11 pages, 4 figures. Paper accepted for Astron. & Astrophy