Massive Stars In The W33 Giant Molecular Complex

Rich in H II regions, giant molecular clouds are natural laboratories to study massive stars and sequential star formation. The Galactic star-forming complex W33 is located at = ∼ ◦ l 12.8 and at a distance of 2.4 kpc and has a size of ≈10 pc and a total mass of ≈(0.8−8.0) × 105 M⊙. The integrated radio and IR luminosity of W33—when combined with the direct detection of methanol masers, the protostellar object W33A, and the protocluster embedded within the radio source W33 main—mark the region as a site of vigorous ongoing star formation. In order to assess the long-term star formation history, we performed an infrared spectroscopic search for massive stars, detecting for the first time 14 early-type stars, including one WN6 star and four O4–7 stars. The distribution of spectral types suggests that this population formed during the past ∼2–4 Myr, while the absence of red supergiants precludes extensive star formation at ages 6–30 Myr. This activity appears distributed throughout the region and does not appear to have yielded the dense stellar clusters that characterize other star-forming complexes such as Carina and G305. Instead, we anticipate that W33 will eventually evolve into a loose stellar aggregate, with Cyg OB2 serving as a useful, albeit richer and more massive, comparator. Given recent distance estimates, and despite a remarkably similar stellar population, the rich cluster Cl 1813–178 located on the northwest edge of W33 does not appear to be physically associated with W33

Glucose effects on gastric motility and tone evoked from the rat dorsal vagal complex

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/66102/1/j.1469-7793.2001.t01-1-00141.x.pd

Carnosine:can understanding its actions on energy metabolism and protein homeostasis inform its therapeutic potential?

The dipeptide carnosine (β-alanyl-L-histidine) has contrasting but beneficial effects on cellular activity. It delays cellular senescence and rejuvenates cultured senescent mammalian cells. However, it also inhibits the growth of cultured tumour cells. Based on studies in several organisms, we speculate that carnosine exerts these apparently opposing actions by affecting energy metabolism and/or protein homeostasis (proteostasis). Specific effects on energy metabolism include the dipeptide's influence on cellular ATP concentrations. Carnosine's ability to reduce the formation of altered proteins (typically adducts of methylglyoxal) and enhance proteolysis of aberrant polypeptides is indicative of its influence on proteostasis. Furthermore these dual actions might provide a rationale for the use of carnosine in the treatment or prevention of diverse age-related conditions where energy metabolism or proteostasis are compromised. These include cancer, Alzheimer's disease, Parkinson's disease and the complications of type-2 diabetes (nephropathy, cataracts, stroke and pain), which might all benefit from knowledge of carnosine's mode of action on human cells. © 2013 Hipkiss et al.; licensee Chemistry Central Ltd

Mycobacterium tuberculosis WhiB3 responds to O2 and nitric oxide via its [4Fe-4S] cluster and is essential for nutrient starvation survival

A fundamental challenge in the redox biology of Mycobacterium tuberculosis (Mtb) is to understand the mechanisms involved in sensing redox signals such as oxygen (O2), nitric oxide (NO), and nutrient depletion, which are thought to play a crucial role in persistence. Here we show that Mtb WhiB3 responds to the dormancy signals NO and O2 through its iron-sulfur (Fe-S) cluster. To functionally assemble the WhiB3 Fe-S cluster, we identified and characterized the Mtb cysteine desulfurase (IscS; Rv3025c) and developed a native enzymatic reconstitution system for assembling Fe-S clusters in Mtb. EPR and UV-visible spectroscopy analysis of reduced WhiB3 is consistent with a one-electron reduction of EPR silent [4Fe-4S]2+ to EPR visible [4Fe-4S]+. Atmospheric O2 gradually degrades the WhiB3 [4Fe-4S]2+ cluster to generate a [3Fe-4S]+ intermediate. Furthermore, EPR analysis demonstrates that NO forms a protein-bound dinitrosyl–iron–dithiol complex with the Fe-S cluster, indicating that NO specifically targets the WhiB3 Fe-S cluster. Our data suggest that the mechanism of WhiB3 4Fe-4S cluster degradation is similar to that of fumarate nitrate regulator. Importantly, Mtb ΔwhiB3 shows enhanced growth on acetate medium, but a growth defect on media containing glucose, pyruvate, succinate, or fumarate as the sole carbon source. Our results implicate WhiB3 in metabolic switching and in sensing the physiologically relevant host signaling molecules NO and O2 through its [4Fe-4S] cluster. Taken together, our results suggest that WhiB3 is an intracellular redox sensor that integrates environmental redox signals with core intermediary metabolism