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Biomedical subjects

J Faris

Publications and source records attributed to J Faris.

12 recordsLinked to original sources

Chromosome mapping and phylogenetic analysis of the cytosolic acetyl-CoA carboxylase loci in wheat.

The cytosolic isoform of plant acetyl-CoA carboxylase is a multidomain enzyme involved in the synthesis of very-long-chain fatty acids and in secondary metabolism. Chromosome mapping of wheat identified one locus containing cytosolic acetyl-CoA carboxylase genes (Acc-2) and a related partially processed pseudogene (Psi-Acc-2) in the distal region of the long arm of wheat homoeologous group 3 chromosomes. Multiple copies of the Acc-2 genes, whose presence was suggested by sequence analysis, are likely to be arranged in tandem repeats. At least three out of five genes cloned from hexaploid wheat map to this locus. Another locus containing Acc-2--related sequences is present in the distal region of the long arm of chromosome 5D. The identity of the hybridizing DNA present at this locus remains unknown. A system based on PCR-cloning and DNA sequence analysis of acetyl-CoA carboxylase genes was developed to address various phylogenetic and systematics questions in grasses. It was applied to reconstruct the phylogeny of the Acc-2 genes from D- and S-genome Aegilops and A-genome Triticum diploid species, AABB- and AAGG-genome tetraploid wheat, and AABBDD-genome hexaploid wheat, as well as from rye and barley. The combined cytogenetic and molecular evolution approach allowed assignment of gene sequences included in phylogenetic analysis to specific loci on homoeologous chromosomes. Recurring gene duplication followed by chromosome translocation and/or possible loss of some gene copies, as well as loss of introns, occurred in the gene family in different plant lineages. Two major Acc-2 clades appeared before the divergence of barley and rye. Nucleotide substitution rates in different parts of the Acc-2 gene were assessed. This analysis of the Acc-2 loci provides detailed information regarding evolutionary events at a low--copy-number locus containing important functional genes. These events are likely to be common and to play a significant role in shaping grass genomes.

Acetyl-CoA Carboxylase↗

Plastid-localized acetyl-CoA carboxylase of bread wheat is encoded by a single gene on each of the three ancestral chromosome sets.

5'-End fragments of two genes encoding plastid-localized acetyl-CoA carboxylase (ACCase; EC 6.4.1.2) of wheat (Triticum aestivum) were cloned and sequenced. The sequences of the two genes, Acc-1,1 and Acc-1,2, are 89% identical. Their exon sequences are 98% identical. The amino acid sequence of the biotin carboxylase domain encoded by Acc-1,1 and Acc-1,2 is 93% identical with the maize plastid ACCase but only 80-84% identical with the cytosolic ACCases from other plants and from wheat. Four overlapping fragments of cDNA covering the entire coding region were cloned by PCR and sequenced. The wheat plastid ACCase ORF contains 2,311 amino acids with a predicted molecular mass of 255 kDa. A putative transit peptide is present at the N terminus. Comparison of the genomic and cDNA sequences revealed introns at conserved sites found in the genes of other plant multifunctional ACCases, including two introns absent from the wheat cytosolic ACCase genes. Transcription start sites of the plastid ACCase genes were estimated from the longest cDNA clones obtained by 5'-RACE (rapid amplification of cDNA ends). The untranslated leader sequence encoded by the Acc-1 genes is at least 130-170 nucleotides long and is interrupted by an intron. Southern analysis indicates the presence of only one copy of the gene in each ancestral chromosome set. The gene maps near the telomere on the short arm of chromosomes 2A, 2B, and 2D. Identification of three different cDNAs, two corresponding to genes Acc-1,1 and Acc-1,2, indicates that all three genes are transcriptionally active.

Acetyl-CoA Carboxylase↗

Effects of mild hypoxia on perceptual-motor performance: a signal-detection approach.

Twelve healthy male subjects were required to make speeded judgements concerning the orientation of visual stimuli while breathing air at reduced partial pressure in a hypobaric chamber at altitudes of 7000 and 12,000 ft. A control condition was also conducted at sea level, and subjects received practice on the task at sea level prior to the commencement of the experiment. Significantly slower response times were obtained at 7000 and 12,000 ft relative to sea level. A signal-detection analysis showed that accuracy of judgement was significantly poorer at 12,000 ft, but oxygen deprivation has no systematic effect on response criterion.

Adult↗

Effects of exposure to simulated altitudes on visual fields, contrast sensitivity, and dazzle recovery.

Previous studies have shown that visual performance may be impaired at altitudes above 12,000 ft when supplementary oxygen is not used. What is not known is whether there may be subtle changes in visual function at altitudes to which airline cabins are usually pressurized. In this study, we measured spatial and temporal contrast sensitivity, central visual field thresholds, and macular photostress recovery time in 12 male subjects at sea level and at simulated altitudes of 7000 ft and 12,000 ft. Our results showed insignificant changes in spatial and temporal contrast sensitivity, central visual field thresholds and dazzle recovery time with respect to simulated altitudes.

Adult↗

Magnetically enhanced coagulation of very small iron grains.

Laboratory experiments, in which very small (approximately 20 nm) grains are produced in the presence of a magnetic field on the order of 100 Gauss in a low-pressure hydrogen atmosphere, have demonstrated that such smokes can become permanently magnetized. We show that magnetization results in an enormous enhancement in the coagulation efficiency of such materials even in the absence of external magnetic fields. Small iron grains should have been produced in the solar nebula by thermal processing of preexisting interstellar grains. If such processing occurred via high-energy electromagnetic events then the resultant magnetized grains could have triggered the formation of centimeter- to meter-sized protoplanetessimals by acting as "nets" capable of sweeping up nonconductive silicates suspended in the gas. It is possible that the presence of conductive fractal aggregates observed in modern-day protostellar disks could be explained by the enhanced coagulation efficiency of very small magnetized iron particles.

Astronomical Phenomena↗