Results 71 to 80 of about 156 (127)

List of seminars for patients M52

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Reports and programs of seminars organized for patient ...
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Abstract list M52

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A yearly list of abstracts of contributions to scientific ...
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Motivation and Satisfaction of Civil Servants: Development of Strategies and Global Experience

open access: yesStudia Ekonomiczne i Regionalne
Lutsenko Оlena   +4 more
doaj   +1 more source

Public report on the performance of the system M52

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Public report on the performance of the system ...
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Periodic report on new media and interactive tools in M52

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Periodic report on new media and interactive tools in ...
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Annual reports on the operational CO2 performance of the system M52

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Annual reports on the operational CO2 performance of the system ...
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Uvby-Beta Photometry of the Open Cluster M52

Publications of the Astronomical Society of the Pacific, 1981
Photometric uvbyβ observations of the open cluster M52 (NGC 7654) are used to determine the cluster's distance modulus (V0 - Mυ = 10.83 ± 0.24) and mean cluster reddening (E(B - V) = 0.57). The likelihood of cluster membership of the F7 Ib supergiant 60°2532 is verified on evolutionary grounds; its absolute magnitude is determined to be Mυ = -4.42 ± 0 ...
S. C. Danford, J. Thomas
exaly   +2 more sources

High-yield cultivation of Marinococcus M52 for production and recovery of hydroxyectoine

Research in Microbiology, 2006
Ectoine and hydroxyectoine, produced by Halomonas ssp. and Marinococcus ssp., have been extensively characterized and proposed for biotechnological applications. Large-scale production of ectoine was achieved by implementing the so-called "milking process" by Bitop (Witten, Germany) and commercializing compatible solutes as stabilizers for biological ...
Chiara Schiraldi   +2 more
exaly   +4 more sources

Photographicuvby photometry of the open cluster M52

Astrophysics and Space Science, 1990
Photographicuvby photometry of 15 stars in the open cluster M52 (NGC 7654) has been obtained. The distance modulusVo−Mv=11.3±0.1 and mean cluster reddeningE(B−V)=0.57 are determined. Some basic physical characteristics of 30 stars with observeduvby values are obtained as well as a numerical estimation of the open cluster age 9.6×107 yr is made.
exaly   +2 more sources

071039 (M52) Stop ‘Stop-loss’ loss

Insurance: Mathematics and Economics, 1995
exaly   +2 more sources

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