# ALBERT

## All Library Books, journals and Electronic Records Telegrafenberg

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• 1
Electronic Resource
[s.l.] : Macmillian Magazines Ltd.
Nature 431 (2004), S. 1069-1072
ISSN: 1476-4687
Source: Nature Archives 1869 - 2009
Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
Notes: [Auszug] The brightness of type Ia supernovae, and their homogeneity as a class, makes them powerful tools in cosmology, yet little is known about the progenitor systems of these explosions. They are thought to arise when a white dwarf accretes matter from a companion star, is compressed and undergoes a ...
Type of Medium: Electronic Resource
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• 2
Electronic Resource
Springer
Journal of molecular evolution 47 (1998), S. 268-274
ISSN: 1432-1432
Keywords: Key words: Synonymous codon usage bias — Estimation methods — Effective number of codons — Codon bias index — Codon adaptation index — Scaled'' χ2— Intrinsic codon bias index
Source: Springer Online Journal Archives 1860-2000
Topics: Biology
Notes: Abstract. Synonymous codons are not generally used at equal frequencies, and this trend is observed for most genes and organisms. Several methods have been proposed and used to estimate the degree of the nonrandom use of the different synonymous codons. The estimates obtained by these methods, however, show different levels of both precision and dispersion when coding regions of a finite number of codons are under analysis. Here, we present a study, based on computer simulation, of how the different methods proposed to evaluate the nonrandom use of synonymous codons are affected by the length of the coding region analyzed. The results show that some of these methods are heavily influenced by the number of codons and that the comparison of codon usage bias between coding regions of different lengths shows a methodological bias under different conditions of nonrandom use of synonymous codons. The study of the dispersion of the estimates obtained by the different methods gives, on the other hand, an indication of the methods to be applied to compare values of codon usage bias among coding regions of equivalent length.
Type of Medium: Electronic Resource
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• 3
Electronic Resource
Springer
Journal of molecular evolution 41 (1995), S. 1152-1159
ISSN: 1432-1432
Keywords: Synonymous substitutions ; Nonsynonymous substitutions ; Estimation methods ; Confidence intervals ; Drosophila
Source: Springer Online Journal Archives 1860-2000
Topics: Biology
Notes: Abstract A method for estimating the numbers of synonymous (Ks) and nonsynonymous (Ka) substitutions per site is proposed. The method is based on the Li's (J Mol. Evol. 36:96–99, 1993) and Pamilo and Bianchi's (Mol. Biol. Evol. 10:271–281, 1993) method, but a putative source of bias is solved. It is proposed that the number of synonymous substitutions that are actually transitions or transversions should be computed by separating the twofold degenerate sites into two types of sites, 2S-fold and 2V-fold, where only transitional and transversional substitutions are synonymous, respectively. Kimura's (J. Mol. Evol. 16:111–120, 1980) two-parameter correcting method for multiple substitutions at a site is then applied using the overall observed synonymous transversion frequency to estimate both the numbers of synonymous transversional (Bs) and transitional (As) substitutions per site. This approach, therefore, also minimizes stochastic errors. Computer simulations indicate that the method presented gives more accurate Ks and Ka estimates than the aforementioned methods. Furthermore, the obtention of confidence intervals for divergence estimates by computer simulation is proposed.
Type of Medium: Electronic Resource
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• 4
Electronic Resource
Springer
Genetica 102-103 (1998), S. 369-382
ISSN: 1573-6857
Keywords: protein evolution ; Drosophila ; synonymous ; nonsynonymous ; Index of Dispersion
Source: Springer Online Journal Archives 1860-2000
Topics: Biology
Notes: Abstract Rates of synonymous and nonsynonymous substitution were investigated for 24 genes in three Drosophila species, D. pseudoobscura, D. subobscura, and D. melanogaster. D. pseudoobscura and D. subobscura, two distantly related members of the obscura clade, differ on average by 0.29 synonymous nucleotide substitutions per site. D. melanogaster differs from the two obscura species by an average of 0.81 synonymous substitutions per site. Using a method developed by Gillespie, we investigated the variance to mean ratio, or Index of Dispersion, R, of substitutions along the three species' branches to test the fundamental prediction of the neutral theory of molecular evolution, E(R) = 1. For nonsynonymous substitutions, the average R, Ra is 1.6, which is not significantly different from the neutral theory prediction. Only 5 of the 24 genes had significantly large Ra valves, and 12 of the genes had Ra estimates of less than one. In contrast, the Index of Dispersion for synonymous substitutions was significantly large for 12 of the 24 genes, with an average of Rs = 4.4, also statistically significant. These findings contrast with results for mammals, which showed overdispersion of nonsynonymous substitutions, but not of synonymous substitutions. Weak selection acting to maintain codon bias in Drosophila, but not in mammals, may be important in explaining the high variance in the rate of synonymous substitutions in this group of organisms.
Type of Medium: Electronic Resource
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• 5
Electronic Resource
Springer
Astrophysics and space science 170 (1990), S. 263-265
ISSN: 1572-946X
Source: Springer Online Journal Archives 1860-2000
Topics: Physics
Notes: Abstract Radial velocities of OB stars are utilised in order to determine the values of some galactic structure parameters in the solar neighbourhood.
Type of Medium: Electronic Resource
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• 6
Electronic Resource
Springer
Astrophysics and space science 187 (1992), S. 187-195
ISSN: 1572-946X
Source: Springer Online Journal Archives 1860-2000
Topics: Physics
Notes: Abstract Some statistical studies on the nearby early-type stars proposed for observations by HIPPARCOS are presented. Results on spatial orientation and kinematics are in agreement with those found in the literature. An age estimate based on non-kinematical hypothesis is found to be somewhat smaller than expansion ages derives by some authors. Finally, it is suggested that Gould's Belt may have formed as a result of high-velocity cloud impact on the galactic disk, and some estimations are presented.
Type of Medium: Electronic Resource
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• 7
Electronic Resource
Springer
ISSN: 1572-9559
Keywords: infrared antennas ; point-contact non-linear devices...
Source: Springer Online Journal Archives 1860-2000
Topics: Physics
Notes: Abstract The electromagnetic coupling between a gaussian beam and whisker structures such as those found in some kinds of non-linear devices used at infrared frequencies is investigated. Calculations show the potential improvement of the electromagnetic coupling coefficient by the proper choice of the focusing angle of the beam and the use of corner reflectors, giving quantitative support to these techniques which have been used for long time.
Type of Medium: Electronic Resource
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• 8
Electronic Resource
Springer
Astrophysics and space science 272 (2000), S. 109-112
ISSN: 1572-946X
Source: Springer Online Journal Archives 1860-2000
Topics: Physics
Notes: Abstract A sample of O- and B-type stars with Hipparcos astrometric data, ages computed from Strömgren photometry and radial velocities, has been used to characterize the structure, age and kinematics of the Gould Belt system. The local spiral structure of our galaxy is determined from this sample, and also from a sample of Hipparcos Cepheid stars. The Gould Belt, with an orientation with respect to the galactic plane ofi G = 16-22° and ΩG =275-295°, extends up to a distance of 600 pc from the Sun. Roughly the 60-65% of the O and B stars younger than 60 Myr in the solar neighbourhood belong to this structure. Our results indicate that the kinematical behaviour of this system is complex, with an expansion motion in the solar neighbourhood (R〈300 pc).In the frame of the Lin's theory, and analysing the O and B stars further than 600 pc and the Cepheids, we found a galactic spiral structure characterized by a 4-arm spiral pattern with the Sun located atψ⊙ = 350-355 ± 30° – near the Sagittarius-Carina arm– and outside the corotation circle. The angular rotation speed of the spiral pattern was found to be Ωp = 31-32 ± 4 kms-1 kpc-1.
Type of Medium: Electronic Resource
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• 9
Publication Date: 2011-01-26
Description: We present a comparison of aerosol properties derived from in situ and remote sensing instruments during DAMOCLES campaign, aimed at investigating the equivalence between the instrumentation and methodologies employed by several Spanish groups to study atmospheric aerosols at a regional background site. The complete set of instruments available during this closure experiment allowed collecting a valuable high-resolution aerosol measurement data set. The data set was augmented with airborne in situ measurements carried out in order to characterize aerosol particles during the midday of 29 June 2006. This work is focused on aerosol measurements using different techniques of high-quality instruments (ground-based remote sensing and aircraft in situ) and their comparisons to characterize the aerosol vertical profiles. Our results indicate that the variability between the detected aerosol layers was negligible in terms of aerosol optical properties and size distributions. Relative differences in aerosol extinction coefficient profiles were less than 20% at 355 and 532 nm and less than 30% at 1064 nm, in the region with high aerosol concentration. Absolute differences in aerosol optical depth (AOD) were below 0.01 at 532 and 1064 nm and less than 0.02 at 355 nm, less than the uncertainties assumed in the AOD obtained from elastic lidar. Columnar values of the lidar ratio revealed some discrepancies with respect to the in situ aircraft measurements, caused fundamentally by the lack of information in the lowest part of the boundary layer.
Print ISSN: 0148-0227
Topics: Geosciences , Physics
Published by Wiley on behalf of American Geophysical Union (AGU).
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• 10
Unknown
Oxford University Press
Publication Date: 2015-05-10
Description: The aim of our study is to use dynamical simulations to explore the influence of two important dynamical bar parameters, bar strength and bar pattern speed on the shape of the bar dust lanes. To quantify the shape of the dust lanes we have developed a new systematic method to measure the dust lane curvature. Previous numerical simulations have compared the curvature of bar dust lanes with the bar strength, predicting a relation between both parameters which has been supported by observational studies but with a large spread. We take into account the bar pattern speed to explore, simultaneously, the effect of both parameters on the dust lane shape. To that end, we separate our galactic bars in fast bars $\left(1 〈 \mathcal {R} 〈 1.4 \right)$ and slow bars $\left(\mathcal {R} 〉 1.4 \right)$ , obtaining, as previous simulations, an inverse relation between the dust lane curvature and the bar strength for fast bars. For the first time, we extend the study to slow bars, finding a constant curvature as a function of the bar strength. As a result, we conclude that weak bars with straight dust lanes are candidates for slow bars. Finally, we have analysed a pilot sample of 10 S 4 G galaxies, obtaining dust lane curvatures lying within the range covered by the simulations.
Print ISSN: 0035-8711
Electronic ISSN: 1365-2966
Topics: Physics
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