Results 191 to 200 of about 3,265 (221)
Structural basis for the cold adaptation of psychrophilic M37 lipase from Photobacterium lipolyticum
Proteins: Structure, Function and Bioinformatics, 2008 The M37 lipase from Photobacterium lipolyticum shows an extremely low activation energy and strong activity at low temperatures, with optimum activity seen at 298 K and more than 75% of the optimum activity retained down to 278 K.
Dae Gwin Jeong +2 more
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Signature of a chemical spread in the open cluster M37
Monthly Notices of the Royal Astronomical Society, 2022 ABSTRACT Recent Gaia photometry of the open cluster M37 has disclosed the existence of an extended main sequence turn-off – like in Magellanic clusters younger than about 2 Gyr – and a main sequence that is broadened in colour beyond what is expected from the photometric errors, at magnitudes well below the region of the extended turn ...
Adriano Pietrinferni +2 more
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Interfacial activation of M37 lipase: A multi-scale simulation study
Biochimica Et Biophysica Acta - Biomembranes, 2017 Lipases are enzymes of biotechnological importance that function at the interface formed between hydrophobic and aqueous environments. Hydrophobic interfaces can induce structural transitions in lipases that result in an increase in enzyme activity, although the detailed mechanism of this process is currently not well understood for many lipases. Here,
Mark S.P. Sansom +2 more
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THE X-RAY LUMINOSITY FUNCTION OF M37 AND THE EVOLUTION OF CORONAL ACTIVITY IN LOW-MASS STARS
Astrophysical Journal, 2016 We use a 440.5 ks Chandra observation of the ≈500-Myr-old open cluster M37 to derive the X-ray luminosity functions of its ≤1.2 M\(\odot\) stars. Combining detections of 162 M37 members with upper limits for 160 non-detections, we find that its G, K, and
Marcel Agüeros, Alejandro Núñez
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Variable Stars in the Open Cluster NGC 2099 (M37) [PDF]
Publications of the Astronomical Society of the Pacific, 2007 Time-series CCD photometric observations of the intermediate-age open cluster NGC 2099 were performed to search for variable stars. We also carried out BV photometry to study physical properties of variables in the cluster. Using V-band time-series data, we carefully examined light variations of about 12,000 stars in the range of 10 < V < 22 mag.
Y B Kang
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Research in Astronomy and Astrophysics, 2018
Abstract The CCD photometric observations of open star cluster M37 (NGC 2099) were carried out up to a limiting magnitude of V ∼ 20 in both B and V filters to search for variable stars using a 2k
Ajaz Ahmad Dar +3 more
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Abstract The CCD photometric observations of open star cluster M37 (NGC 2099) were carried out up to a limiting magnitude of V ∼ 20 in both B and V filters to search for variable stars using a 2k
Ajaz Ahmad Dar +3 more
exaly +2 more sources
Alloy Digest, 2004
Abstract Wieland-M37 has excellent cold-working properties and corrosion resistance. The alloy is used in the deep-drawn and stamped condition for electrical products. This datasheet provides information on composition, physical properties, microstructure, hardness, elasticity, and tensile properties.
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Abstract Wieland-M37 has excellent cold-working properties and corrosion resistance. The alloy is used in the deep-drawn and stamped condition for electrical products. This datasheet provides information on composition, physical properties, microstructure, hardness, elasticity, and tensile properties.
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2023
The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements. They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
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The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements. They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
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Photometric study of an eclipsing binary in the field of M37
Research in Astronomy and Astrophysics, 2014CCD photometric observations with B and V passbands were performed on the contact binary V3 in the field of open cluster M37. The solutions were obtained for data from both B and V passbands along with R passband given by Hartman et al. using the Wilson-Devinney code.
Devarapalli Shanti Priya +2 more
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VFF_D0.2 Final Report (M37-M42)
2013This deliverable is organized through different sections meant to give a complete perspective on the VFF activities accomplished within the months between 37 and 42 of the project (Sept. 2012 - Feb. 2013). This paragraph will introduce the VFF objectives as they can be derived from the DoW, while the following sections will describe the work done to ...
Sacco M., Redaelli C.
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