The stimulatory effects of eNOS/F92A-Cav1 on NO production and angiogenesis in BMSCs

Nitric oxide (NO) is generated in endothelial cells by endothelial nitric oxide synthase (eNOS). Caveolin-1 (Cav1) inhibits eNOS function and NO production. Modifying Cav1 scaffold domain, in particular Phenylalanine at position 92 (F92) is critical for the inhibitory actions of Cav1 toward eNOS. The aims of this study were to investigate the effect of enhanced NO production in term of in vitro angiogenesis on rat bone marrow derived mesenchymal stem cells (BMSCs) transduced with a novel bicistronic lentiviral vector co-expressing eNOS and mutant Cav1 (F92A). METHODS: A bicistronic eNOS/F92-Cav1 lentiviral vector was constructed, and used to transduce rat BMSCs. The expression of eNOS and VEGF protein were confirmed by western-blot. NO production was detected by the greiss assay and in vitro angiogenesis was assessed by matrigel assisted capillary tube formation. The cell viability was evaluated using a Cell Counting Kit (CCK)-8. RESULTS: The bicistronic eNOS/F92A-Cav1 lentiviral vector increased eNOS and VEGF protein expression, NO production compared to controls. In vitro capillary formation was increased in eNOS-F92A transduced cells and cell viability was not affected by transduction. CONCLUSION: Transduction of rat BMSCs with an eNOS-F92A-Cav1 lentiviral vector can increase NO production by enhancing eNOS protein expression. The increased NO production did not reduce cell viability. This study demonstrates that genetic modification of BMSCs to enhance NO producton could be applied in stem cell based therapeutic approaches to treat diseases such as pulmonary arterial hypertension (PAH) which is characterized by decreased endothelial NO release

SCOPE: SCUBA-2 Continuum Observations of Pre-protostellar Evolution - survey description and compact source catalogue

We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consists of 850 μm continuum observations of 1235 Planck Galactic Cold Clumps (PGCCs) made with the Submillimetre Common-User Bolometer Array 2 on the James Clerk Maxwell Telescope. These data are at an angular resolution of 14.4 arcsec, significantly improving upon the 353 GHz resolution of Planck at 5 arcmin, and allowing for a catalogue of 3528 compact sources in 558 PGCCs. We find that the detected PGCCs have significant sub-structure, with 61 per cent of detected PGCCs having three or more compact sources, with filamentary structure also prevalent within the sample. A detection rate of 45 per cent is found across the survey, which is 95 per cent complete to Planck column densities of N(H2) > 5 × 10^21 cm^−2. By positionally associating the SCOPE compact sources with young stellar objects, the star formation efficiency, as measured by the ratio of luminosity to mass, in nearby clouds is found to be similar to that in the more distant Galactic Plane, with the column density distributions also indistinguishable from each other