Search results for "HIF"

showing 10 items of 1515 documents

Gaia DR2 reveals a star formation burst in the disc 2-3 Gyr ago

2019

We use Gaia DR2 magnitudes, colours and parallaxes for stars with G<12 to explore a 15-dimensional space that includes simultaneously the initial mass function (IMF) and a non-parametric star formation history (SFH) for the Galactic disc. This inference is performed by combining the Besancon Galaxy Model fast approximate simulations (BGM FASt) and an approximate Bayesian computation algorithm. We find in Gaia DR2 data an imprint of a star formation burst 2-3 Gyr ago, in the Galactic thin disc domain, and a present star formation rate (SFR) of about 1 Msun. Our results show a decreasing trend of the SFR from 9-10 Gyr to 6-7 Gyr ago. This is consistent with the cosmological star formation …

Stellar massFOS: Physical sciencesPerturbation (astronomy)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsmass function -galaxiesstar formation rate01 natural sciencesdisk -Galaxy0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicsluminosity functionDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsstellar content -Hertzsprung-Russell and C-M diagramsstars010308 nuclear & particles physicsStar formationDiscos (Astrofísica)Astronomy and Astrophysicsstellar initial mass functioninteractionsGalaxiesAstrophysics - Astrophysics of GalaxiesStarsGalaxyRedshiftevolution -Galaxystar formation historyGalàxiesEstelsStarsGalaxyGalaxies evolutionDisks (Astrophysics)[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)galaxy mergeEvolució de les galàxiesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Lyman break and ultraviolet-selected galaxies at z ~ 1 - II. PACS 100μm/160μm FIR detections

2013

In this work, we report the Photodetector Array Camera and Spectrometer (PACS) 100 μm/160 μm detections of a sample of 42 GALEX-selected and far-infrared (FIR)-detected Lyman break galaxies (LBGs) at z ~ 1 located in the Cosmic Evolution Survey (COSMOS) field and analyse their ultraviolet (UV) to FIR properties. The detection of these LBGs in the FIR indicates that they have a dust content high enough so that its emission can be directly detected. According to a spectral energy distribution (SED) fitting with stellar population templates to their UV-to-near-IR observed photometry, PACS-detected LBGs tend to be bigger (Reff ~ 4.1 kpc), more massive [log (M*/M⊙) ~ 10.7], dustier [Es(B - V) ~ …

Stellar populationAstrophysicsgalaxies [Radio continuum]medicine.disease_causestar formation [Galaxies]Physical cosmologyhigh-redshift [Galaxies]galaxies [Infrared]galaxies: high-redshiftmedicineLuminous infrared galaxyPhysicsStar formationinfrared: galaxieAstronomyAstronomy and Astrophysicsevolution [Galaxies]RedshiftGalaxygalaxies [Ultraviolet]Space and Planetary Sciencegalaxies: star formationultraviolet: galaxiesSpectral energy distributionradio continuum: galaxiegalaxies: evolutionUltraviolet
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Preferential azido bridging regulating the structural aspects in cobalt(III) and copper(II)–Schiff base complexes: Syntheses, magnetostructural corre…

2011

International audience; A tridentate NNO donor Schiff base ligand [(1Z,3E)-3-((pyridin-2-yl)methylimino)-1-phenylbut-1-en-1-ol = LH] in presence of azide ions coordinates with cobalt(II) and copper(II) ions giving rise to three new coordination complexes [Co2(L)2(μ1,1-N3)2(N3)2] (1), [Cu2(L)2(μ1,3-N3)]·ClO4 (2) and [(μ1,1-N3)2Cu5(μ-OL)2(μ1,1-N3)4(μ1,1,1-N3)2]n (3). The complexes have been characterized by elemental analysis, FT-IR, UV–Vis spectral studies, and single crystal X-ray diffraction studies. These complexes demonstrate that under different synthetic conditions the azide ions and the Schiff base ligand (LH) show different coordination modes with cobalt(II) and copper(II) ions, givi…

Stereochemistry1chemistry.chemical_elementCrystal structure[CHIM.INOR]Chemical Sciences/Inorganic chemistry010402 general chemistry01 natural sciencesCatalysisInorganic Chemistrychemistry.chemical_compoundMaterials Chemistry[CHIM.CRIS]Chemical Sciences/Cristallography[CHIM]Chemical SciencesPhysical and Theoretical Chemistrychemistry.chemical_classification1-Schiff base010405 organic chemistryAlkene3-Azide[CHIM.MATE]Chemical Sciences/Material chemistryCopper0104 chemical sciencesCrystallographyCuII Schiff basechemistryVTM Alkene oxidationCrystal structuresM = CoIIIAzideμ1Single crystalCobalt
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Multinuclear magnetic resonance and x-ray diffraction studies of aminonitropyridines

1992

The 15N NMR spectra for 21 aminonitropyridines were measured and their chemical shifts assigned. The 1H and 13C NMR chemical shifts and spin–spin coupling constants were also determined for 16 compounds of this series. In order to relate the structural properties of nitramino groups and their 15N NMR chemical shifts in 2- and 4-nitramino-3-nitropyridines, which differ remarkably from all other amino groups studied, low-temperature 1H NMR, 17O NMR, comparative INEPT and IR spectroscopic studies were carried out. In addition, the x-ray crystal structure of 2-nitramino-3-nitropyridine was determined. Comparative spectroscopic studies showed that the nitramino derivatives exhibit different char…

StereochemistryCarbon-13 NMR satelliteChemical shiftGeneral ChemistryNuclear magnetic resonance spectroscopyCarbon-13 NMRTautomerNMR spectra databasechemistry.chemical_compoundCrystallographychemistryProton NMRGeneral Materials SciencePyridiniumMagnetic Resonance in Chemistry
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1H,13C and15N NMR spectroscopic, x-ray structural andab initio/HF studies on nitramino andN-alkylamino-4-nitro derivatives of pyridineN-oxides and py…

2003

The 1H, 13C and 15N NMR spectra in DMSO-d6 were measured for eight nitraminopyridine N-oxides, ten 4-nitropyridine N-oxides, four 2-nitraminopyridines and five 4-nitropyridines. Their chemical shift assignments are based on PFG 1H,X (X = 13C and 15N) HMQC and HMBC experiments. The relative energies for the tautomers of two nitraminopyridine N-oxides were determined by ab initio HF/6–311G** calculations. A single-crystal x-ray structural analysis was made for 4-methyl-2-nitraminopyridine: C6H7O2N3, M = 153.15, triclinic, space group P-1 (No. 2), a = 7.0275(4), b = 6.8034(3), c = 8.6086(5) A, α = 103.620(2), β = 90.309(2), γ = 122.215(3)°, V = 334.11(3) A3, Z = 2. Copyright © 2003 John Wiley …

StereochemistryChemical shiftAb initioGeneral ChemistryCarbon-13 NMRTriclinic crystal systemTautomerNMR spectra databasechemistry.chemical_compoundCrystallographychemistryPyridineProton NMRGeneral Materials ScienceMagnetic Resonance in Chemistry
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Über polygermane

1984

Abstract The optimum conditions for selectively cleaving off two phenyl groups in Ge2Ph6 by trichloroacetic acid have been determined. Neither trihaloacetic acids nor HCl/AlCl3 nor reactive tetrahalides MCl4 are suitable reagents for cleaving one phenyl group alone. The 13C NMR chemical shifts of functional phenyl-mono- and -digermanes are given. The crystal structure of 1,2-bis(trichloroacetate)tetraphenyldigermane has been determined and refined to R = 0.048. The digermane bond is bridged by both acetates (distances GeGe 239.3(2), GeO 207.3(3) and 231.4(3) pm). The Ge atoms have trigonal bipyramidal coordination.

StereochemistryChemical shiftOrganic ChemistryCrystal structureNuclear magnetic resonance spectroscopyCarbon-13 NMRBiochemistryMedicinal chemistryInorganic ChemistryTrigonal bipyramidal molecular geometrychemistry.chemical_compoundchemistryMaterials ChemistryPhenyl groupMoleculePhysical and Theoretical ChemistryDigermaneJournal of Organometallic Chemistry
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13C and15N NMR chemical shift assignments ofN-1-(2- azidoethyl)-4-R-pyrimidin-2-ones by1H,X HMQ(B)C withz-gradient selection

1998

13C and 15N NMR chemical shift assignments based on z-gradient selected 1H,X (X=13C and 15N) HMQC and HMBC experiments are reported for N-1-(2-azidoethyl)pyrimidin-2-one (ring system of cytosine), its five 4-R derivatives [where R=NH2, OCH3, N(CH2)4, NHCH2CH(CH3)2 and N(CH3)2] and 2-azidoethyl tosylate. The possibilities of detecting all nitrogens in these molecules containing (i) an azido group at N-1 and (ii) an electronegative substituent at C-4 are limited. First, the terminal nitrogen of the azido group is difficult to observe because the nearest proton (in a CH2 group) is located four bonds away from it. Second, in contrast to N-1, N-3 in N-1-(2-azido-ethyl)-4-pyrimidin-2-ones remaine…

StereochemistryChemical shiftSubstituentGeneral ChemistryCarbon-13 NMRRing (chemistry)chemistry.chemical_compoundchemistryGroup (periodic table)Proton NMROrganic chemistryMoleculeGeneral Materials ScienceCytosineMagnetic Resonance in Chemistry
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Nitramino, NRNO2 (R = H, CH3), as a substituent.13C and15N NMR spectroscopic study of nitraminobenzenes and -pyridines

1993

In order to clarify the special properties of the aryl-bound nitramino substituent NRNO 2 (R=H, CH 3 ), 13 C and 15 N NMR spectra of six nitraminobenzenes and nine nitraminopyridines were measured in DMSO-d 6 and their chemical shifts assigned. 1 H NMr chemical shifts and spin-spin coupling constants of all the compounds were also determined. In contrast to the behaviour of nitropyridines or -benzenes studied previously, most of the present compounds gave very broad 17 O NMR lines even at elevated temperatures and their 17 O NMR data were not useful for any reliable conclusions

StereochemistryChemical shiftSubstituentGeneral ChemistryNuclear magnetic resonance spectroscopyNmr dataMedicinal chemistryNMR spectra databasechemistry.chemical_compoundchemistryBenzene derivativesProton NMRNitroamineGeneral Materials ScienceMagnetic Resonance in Chemistry
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Specificity of 15N NMR chemical shifts to the nature of substituents and tautomerism in substituted pyridine N-oxides

2012

1H, 13C, and 15N NMR chemical shifts have been measured for 2-aminopyridine N-oxide (1), its eleven derivatives (2–10, 13, 14), and 3-Cl and 3-Br substituted 4-nitropyridine N-oxides (11, 12). δ(15N) of pyridine ring nitrogen in 2-acetylaminopyridine N-oxides are 5.9–11.5 ppm deshielded from those in 2-aminopyridine N-oxides. When amino and acetylamino substituents are in 4-position, δ(15N) of ring nitrogen is 21.3 ppm deshielded in the acetylated derivative. The strong resonance interaction between 2-amino and 5-nitro groups reflects in the decrease of amino nitrogen shielding about 5.3–17.9 ppm. Also, 1H and 13C NMR spectral data are in agreement with 15N NMR results reflected as deshield…

StereochemistryChemical shiftchemistry.chemical_elementCarbon-13 NMRCondensed Matter PhysicsRing (chemistry)Resonance (chemistry)NitrogenMedicinal chemistryTautomerchemistry.chemical_compoundchemistryPyridinePhysical and Theoretical ChemistrySpectral dataStructural Chemistry
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On heterocyclic systems containing bismuth(III) 2. Eight-membered heterocycles Cl/Br/I-M(CH2CH2CH2)2X with lewis acidic group 15 atoms M  As, Sb, Bi…

1994

Abstract Paths to the ligands (Cl/Br-CH2CH2CH2)2NR/O/S/Se, R  Me, Bz, iPr, iBu, to the diGrignard reagents (Cl/BrMg-CH2CH2CH2)2NR/O/S, R  Me, Bz, iPr, iBu and to the eight-membered group 15 heterocycles (Cl/Br/I-As/Sb/Bi(CH2CH2CH2)2NR/S, R  Me, Bz, iBu are given. 13C-NMR, IR and Raman spectra are discussed; for the compound ClSb(CH2CH2CH2)2NMe the crystal structure analysis is given : the antimony atom is clearly Lewis acidic with ψ-trigonal-bipyramidal coordination and a transannular Sb⋯N interaction of 2.385(2) A. For such a configuration the values of the 13C-NMR chemical shifts of the α-CH2-groups (e.g. Cl-As/Sb/Bi(αCH2CH2CH2)2NMe 34.6, 25.9, 46.6 ppm) display clearly a sequence N > …

StereochemistryChemical shiftchemistry.chemical_elementCrystal structureBismuthInorganic ChemistryElectronegativityCrystallographysymbols.namesakechemistryAntimonyReagentAtomMaterials ChemistrysymbolsPhysical and Theoretical ChemistryRaman spectroscopyPolyhedron
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