Search results for "Planetary Science"

showing 10 items of 4367 documents

Informe de la Societat Valenciana de Psicologia amb relació al Decret de plurilingüisme de la Generalitat Valenciana

2018

Artículo:PSICOLOGÍA [UNESCO]General Earth and Planetary SciencesUNESCO::PSICOLOGÍAGeneral Environmental ScienceAnuari de Psicologia de la Societat Valenciana de Psicologia
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Présence d’Asellides stygobies (Crustacea, Isopoda, Aselloidea) dans la région du Primorye, Sibérie sud-orientale

1993

Two species of anophthalmous, unpigmentedasellids have been found in springs and groundwaters of S.E. Siberia (Primorye region). Asellus (Asellus) primoryensis n. sp. is closelyrelated to the epigean species A. (A.) hilgendorfii Bovallius, 1886, as is the case for all stygobiont Asellus (Asellus) species previously known from the Japanese archipelago. Sibirasellus parpurae n. g., n. sp. is closely related to the microphthalmous species Asellus dentifer Birstein & Levanidov, 1952 from the Ussuri Basin (Khor region), now type-species of the new genus Sibirasellus. These two species show several original characters: body covered by numerous cuticular squamulae, mandibular palp reduced (gla…

Asellusgeographygeography.geographical_feature_categoryEcologymedia_common.quotation_subjectBiogeographyBiologybiology.organism_classificationstygobiont asellidsCoalescent theorytaxonomyFar East and Pacific North AmericaGenusArchipelagoGeneral Earth and Planetary SciencesTaxonomy (biology)SubgenusPhyletic gradualismbiogeographyGeneral Environmental Sciencemedia_common
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Association for Moral Education (AME)

2018

Association for Moral Education (AME) Artículo:PSICOLOGÍA [UNESCO]General Earth and Planetary SciencesUNESCO::PSICOLOGÍAAssociation (psychology)PsychologyMoral educationGeneral Environmental ScienceDevelopmental psychologyAnuari de Psicologia de la Societat Valenciana de Psicologia
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Oxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

2011

Context: Dark cloud chemical models usually predict large amounts of O2, often above observational limits. Aims: We investigate the reason for this discrepancy from a theoretical point of view, inspired by the studies of Jenkins and Whittet on oxygen depletion. Methods: We use the gas-grain code Nautilus with an up-to-date gas-phase network to study the sensitivity of the molecular oxygen abundance to the oxygen elemental abundance. We use the rate coefficient for the reaction O + OH at 10 K recommended by the KIDA (KInetic Database for Astrochemistry) experts. Results: The updates of rate coefficients and branching ratios of the reactions of our gas-phase chemical network, especially N + C…

AstrochemistryChemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Analytical chemistrychemistry.chemical_elementFOS: Physical sciencesAstrophysicsAstrophysicsKinetic energy01 natural sciencesOxygen[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesSolar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010304 chemical physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Molecular cloudAstronomy and Astrophysicsastrochemistry; ISM; abundances; ISM; molecules; ISM; individual objects; L134N; ISM; individual objects; TMC-1[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]NitrogenchemistryAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceMolecular oxygenChemical network
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The hyperfine structure in the rotational spectrum of CF+

2012

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter lines. The origin of this double-peak profile may be kinematic or spectroscopic. Aims. We investigate the effect of hyperfine interactions due to the fluorine nucleus in CF+ on the rotational transitions. Methods. We compute the fluorine spin rotation constant of CF+ using high-level quantum chemical methods and determine the relative positions and intensities of each hyperfine component. This information is used to fit the theoretical hyperfine components to the observed CF+ line profiles, thereby employing the h…

AstrochemistryFOS: Physical sciencesContext (language use)Astrophysics010402 general chemistryRotation01 natural sciencesISM: clouds0103 physical sciencesSpin (physics)010303 astronomy & astrophysicsHyperfine structureAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsNebularadio lines: ISMastrochemistryAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesISM: molecules0104 chemical sciences[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ISM: individual objects: Horsehead nebula[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Atomic physicsBar (unit)
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A KInetic Database for Astrochemistry (KIDA)

2012

We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be vetted to the greatest extent possible. Submissions of measured and calculated rate coefficients are welcome, and will be studied by experts before inclusion into the database. Besides providing kinetic information for the interstellar medium, KIDA is planned to contain such data for planetary atmospheres and for circumstellar envelopes. Each year, a subset of the reactions in the database (kida.uva) will be provided as a network for the simulation of the chemistry of dense…

Astrochemistry[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Interstellar cloudFOS: Physical sciencesAstrophysicsKinetic energycomputer.software_genreAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesmiscellaneous [astrochemistry; astronomical databases]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010304 chemical physicsDatabaseKinetic informationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesInterstellar mediumSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)computerChemical databaseGalaxy Astrophysics
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Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity

2021

We perform magnetohydrodynamic simulations of accreting, equal-mass binary black holes in full general relativity focusing on the impact of black hole spin on the dynamical formation and evolution of minidisks. We find that during the late inspiral the sizes of minidisks are primarily determined by the interplay between the tidal field and the effective innermost stable orbit around each black hole. Our calculations support that a minidisk forms when the Hill sphere around each black hole is significantly larger than the black hole's effective innermost stable orbit. As the binary inspirals, the radius of the Hill sphere decreases, and minidisk sconsequently shrink in size. As a result, ele…

Astrofísica010504 meteorology & atmospheric sciencesGeneral relativityastro-ph.GAgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLuminosityGravitationGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsMass ratioAstrophysics - Astrophysics of Galaxies3. Good healthBlack holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Hill sphereAstronomiaAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Absolute kinematics of radio-source components in the complete S5 polar cap sample: IV. Proper motions of the radio cores over a decade and spectral …

2016

We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the source cores up to a few micro-arcseconds per year. The observations were performed at 14.4 GHz and 43.1 GHz, and enable us to estimate the frequency core-shifts in a subset of sources, for which the spectral-index distributions can be computed. We study the source-position stability by analysing the changes in the relative positions of fiducial source points (the jet cores) ove…

AstrofísicaActive galactic nucleusAstrometriaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematics01 natural sciencesStability (probability)Radio continuum: generalBinary black hole0103 physical sciencesVery-long-baseline interferometry010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)general [Radio continuum]general [BL Lacertae objects]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsgeneral [Quasars]BL Lacertae objects: generalAstrometryAstrometryAstrophysics - Astrophysics of GalaxiesQuasars: generalGravitational lensSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]Astrophysics - Instrumentation and Methods for Astrophysics
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The gamma-ray emitting radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447 I. The X-ray View

2015

As part of the TANAMI multiwavelength progam, we discuss new X-ray observations of the $\gamma$-ray and radio-loud Narrow Line Seyfert galaxy ($\gamma$-NLS1) PKS 2004-447. The active galaxy is a member of a small sample of radio-loud NLS1s detected in $\gamma$-rays by the Fermi Large Area Telescope. It is the radio-loudest and only southern-hemisphere source in this sample. We present results from our X-ray monitoring program comprised of Swift snapshot observations from 2012 through 2014 and two new X-ray observations with XMM-Newton in 2012. We analyze the X-ray spectrum and variability of this peculiar source using supplementary archival data from 2004 and 2011. The (0.5-10) keV spectrum…

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumlaw.inventionTelescopeRelativistic beaminglaw0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsMonitoring programAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)AstronomiaComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies throug…

2021

Full list of authors: Baldi, R. D.; Williams, D. R. A.; Beswick, R. J.; McHardy, I.; Dullo, B. T.; Knapen, J. H.; Zanisi, L.; Argo, M. K.; Aalto, S.; Alberdi, A.; Baan, W. A.; Bendo, G. J.; Fenech, D. M.; Green, D. A.; Klöckner, H. -R.; Körding, E.; Maccarone, T. J.; Marcaide, J. M.; Mutie, I.; Panessa, F.; Pérez-Torres, M. A.; Romero-Cañizales, C.; Saikia, D. J.; Saikia, P.; Shankar, F.; Spencer, R. E.; Stevens, I. R.; Uttley, P.; Brinks, E.; Corbel, S.; Martí-Vidal, I.; Mundell, C. G.; Pahari, M.; Ward, M. J.

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical Phenomenanuclei [galaxies]jets [galaxies]Doubly ionized oxygenFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesLuminosityAstrophysical jetSubatomic Physics0103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsConnection (algebraic framework)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxies: nucleiAstronomia ObservacionsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Galaxies: star formation010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxies: activeAstrophysics - Astrophysics of Galaxiesgalaxies [radio continuum]Accretion (astrophysics)Galaxy[SDU]Sciences of the Universe [physics]Meteorology and Atmospheric SciencesSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)active [galaxies]Production (computer science)star formation [galaxies]Astrophysics - High Energy Astrophysical Phenomena
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