Parameters of very young and massive stars with dust shells

A radiative transfer model for newly formed hot stars surrounded by optically thick dust shells is applied to a number of compact infrared sources. The model parameters are derived by fitting the synthetic spectra to the observed one between 8 and 13 m and used to derive additional properties of the shells and the embedded stars.     

Measurements of PM<Subscript>10</Subscript> ions and trace gases with the online system MARGA at the research station Melpitz in Germany – A five-year study

An hourly quantification of inorganic water-soluble PM₁₀ ions and corresponding trace gases was performed using the Monitor for AeRosols and Gases in ambient Air (MARGA) at the TROPOS research site in Melpitz, Germany. The data availability amounts to over 80% for the five-year measurement period from 2010 to 2014. Comparisons were performed for the evaluation of the MARGA, resulting in coefficients of determinations (slopes) of 0.91 (0.90) for the measurements against the SO₂ gas monitor, 0.84 (0.88), 0.79 (1.39), 0.85 (1.20) for the ACSM NO₃ ^?, SO₄ ^2? and NH₄ ⁺ measurements, respectively, and 0.85 (0.65), 0.88 (0.68), 0.91 (0.83), 0.86 (0.82) for the filter measurements of Cl^?, NO₃ ^?, SO₄ ^2? and NH₄ ⁺, respectively. A HONO comparison with a batch denuder shows large scatter (R² = 0.41). The MARGA HNO₃ is underestimated compared to a batch and coated denuder with shorter inlets (slopes of 0.16 and 0.08, respectively). Less NH₃ was observed in coated denuders for high ambient concentrations. Long-time measurements show clear daily and seasonal variabilities. Potential Source Contribution Function (PSCF) analysis indicates the emission area of particulate ions Cl^?, NO₃ ^?, SO₄ ^2?, NH₄ ⁺, K⁺ and gaseous SO₂ to lie in eastern European countries, predominantly in wintertime. Coarse mode sea salt particles are transported from the North Sea to Melpitz. The particles at Melpitz are nearly neutralised with a mean molar ratio of 0.90 for the five-year study. A slight increase of the neutralization ratio over the last three years indicates a stronger decrease of the anthropogenically emitted NO₃ ^? and SO₄ ^2? compared to NH₄ ⁺.     

Incorporation of trivalent actinides into calcite: A time resolved laser fluorescence spectroscopy (TRLFS) study

In order to characterize and quantify the substitution of Ca(II) by Cm(III) (coordination, charge compensation), homogeneous Cm(III) coprecipitated calcite was synthesized in a mixed-flow-through experiment. Two sets of experiments were conducted at pH 8.1 and at pH 12.5.At pH 8.1 two calcites, a calcite with a low Cm³⁺ concentration (LCMpH8.1) and a calcite with a high M³⁺ (Gd³⁺ and Cm³⁺) concentration (HCMpH8.1) were grown and investigated by time resolved laser fluorescence spectroscopy. The Cm(III) emission spectra of LCMpH8.1 and HCMpH8.1 show the same Cm(III) fluorescence signals for two Cm(III) species; Cm(III) species (1) with a peak maximum at 606.2 nm and Cm(III) species (2) with a peak maximum at 620.3 nm. Cm(III) species (1) has a mean lifetime of τ = 386 ± 40 μs and Cm(III) species (2) has a mean lifetime of τ = 1874 ± 200 μs. A lifetime of 386 μs correlates with 1.3 water molecule in the first coordination sphere of the Cm ion whereas a lifetime of 1874 μs indicates the total loss of the Cm(III) hydration sphere. According to the fluorescence emission peak position and the fluorescence emission lifetime, Cm(III) species (1) is identified as a surface sorbed species whereas Cm(III) species (2) is identified as a Cm(III) incorporated into the calcite lattice.Cm(III) fluorescence emission spectra of Cm(III) doped calcite grown at pH 12.5 (LCMpH12.5) show the same peak maxima which are found for LCMpH8.1 and HCMpH8.1 grown at pH 8.1 but an additional emission band at 608.2 nm (3) is found, which can be assigned to a further Cm(III) species. Fluorescence emission lifetime measurements show that this Cm(III) species (3) has a lifetime of τ = 477 ± 25 μs, which correlates with 0.9 water molecules in the first coordination sphere. Cm(III) species (3) is suggested to be a CmOH²⁺ incorporated species.     

Geophysical, geotechnical and hydrological investigations of a small landslide in the French Alps

Geophysical, geotechnical and hydrological surveys were conducted in the French Alps on a small landslide in black marl material to assess the stability. The geophysical survey, consisting of electromagnetic, geo-electric and relative differences in water content.

The data on the basal slip surface, together with geotechnical parameters (cohesion and angle of internal friction), were used to make a stability analysis. This analysis revealed that a groundwater level of 4 m below the ground surface is the critical threshold for reactivating the landslide.

The hydrological investigation, which entailed measurements of saturated permeability and pressure heads, indicated that instability depended on long-term wet conditions with little evapotranspiration.     

Solubility of HOCl in water and aqueous H2SO4 to stratospheric temperatures

Henry's law constants K_H (mol kg^–1 atm^–1) for the reaction HOCl_(g)=HOCl_(aq) near room temperature, literature data for the associated enthalpy change, and solubilities of HOCl in aqueous H₂SO₄ (46 to 60 wt%) at temperatures relevant to the stratosphere (200 KT230 K) are shown to be thermodynamically consistent. Effective Henry's law constants [H*=mHOCl/pHOCl, in mol kg^–1 atm^–1] of HOCl in aqueous H₂SO₄ are given by: ln(H*)=6.4946–mH₂SO₄(–0.04107+54.56/T)–5862 (1/T_o–1/T) where T(K) is temperature and T_o=298.15K. The activity coefficient of HOCl in aqueous H₂SO₄ has a simple Setchenow-type dependence upon H₂SO₄ molality.     

Age,origin and geodynamic significance of a polymetamorphic felsic intrusion in the Ötztal Crystalline Basement,Tirol, Austria

Summary A multi-method approach was applied to derive the age and origin of an orthogneiss body located in the central Kaunertal, western Ötztal Crystalline Basement (ÖCB). The Tieftal orthogneiss body is an internally differentiated, polymetamorphosed epizonal intrusion, embedded in amphibolites. It comprises leucocratic hedenbergite-hornblende-, hornblende- and biotite-hornblende-gneisses, but also some melanocratic rock types. The leucocratic Tieftal gneisses are granitic, have a near eutectic melt composition and share some features of A-type granites, such as high Na₂O+K₂O(8.07 to 8.58wt%), Zr (379 to 554ppm) and Y (58 to 79ppm) contents. The REE-patterns are rather flat ((La/Yb)_N=2.4 to 3.7), with distinct negative Eu anomalies. Single zircon evaporation dating of two samples and Sm-Nd dating of relict magmatic titanite resulted in ages of 487±7, 484±3 and 487±5Ma, respectively. The weighted mean of 485±3Ma is interpreted as the primary crystallization age of the Tieftal orthogneiss body. Rb-Sr whole rock dating results in a well defined regression line, corresponding to an age of 411±9Ma. This age clearly documents at least a partial resetting of the whole rock Rb-Sr system, which is most probably due to subsequent metamorphic overprint. The leucocratic Tieftal gneisses are isotopically rather primitive with an Nd _CHUR ^{485 Ma} value of +1.7 and a calculated magmatic initial⁸⁷Sr/⁸⁶Sr ratio of 0.7047. These data suggest a major mantle contribution. Most probably, they originated through fractionation of the magmatic precursors of the accompanying tholeiitic metabasites. The more primitive isotopic composition of ÖCB metabasites and some late Archean/early Proterozoic and Cambrian inheritance in Tieftal gneiss zircons suggest some involvement of old crustal rocks, too. The amount of crustal contamination can be calculated to be in the range of 10 to 40%. The Tieftal gneisses and the accompanying metabasites are interpreted as remnants of igneous rocks related to an early Ordovician rifting and incipient formation of new oceanic crust, an event which can be traced throughout the central and western European Variscan and Alpine terranes.

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Alter, Genese und geologische Bedeutung einer polymetamorphen felsischen Intrusion im Ötztalkristallin, Tirol, Österreich

Zusammenfassung Ein Vielzahl von Methoden wurde angewandt, um das Alter und die Genese eines Orthogneiskörpers im mittleren Kaunertal, westliches Ötztalkristallin, abzuleiten. Der Tieftal-Orthogneiskörper ist eine in Amphiboliten eingeschaltete, intern differenzierte, polymetamorph überprägte, epizonale Intrusion. Er umfaßt sowohl leukokrate Hedenbergit-Hornblende-, Hornblende- und Biotit-Hornblende-Gneise als auch untergeordnet melanokrate Gesteine. Die leukokraten Tieftal-Gneise besitzen einen granitischen, beinahe einer eutektischen Schmelze entsprechenden Chemismus; einige Parameter wie hohe Na₂O+K₂O(8.07 bis 8.58Gew%), Zr(379 bis 554ppm) und Y(58 bis 79ppm) Gehalte weisen auf eine A-Typ Affinität hin. Die SEE-Spektren sind nur gering fraktioniert ((La/Yb)_N=2.3 bis 3.7) und weisen eine markante negative Eu-Anomalie auf. Einzelzirkon-Evaporationsdatierungen an 2 Proben und eine Sm-Nd Datierung von reliktischem magmatischem Titanit ergeben Alter von 487±7, 484±3 und 487±5Ma. Der gewichtete Mittelwert von 485±3Ma wird als das primäre magmatische Kristallisationsalter des Tieftal-Orthogneiskörpers interpretiert. Eine Rb-Sr Gesamtgesteinsdatierung ergibt eine gut definierte Regressionsgerade mit einem Alter von 411±9Ma. Dieses Alter beweist eine postmagmatische Störung des Rb-Sr Gesamtgesteinssystems, die durch die metamorphen überprägungen verursacht wurde. Die leukokraten Tieftal-Gneise besitzen eine relative primitive isotopische Zusammensetzung mit einem Nd _CHUR ^{485 Ma} a Wert von +1.7 und einem zurückgerechneten magmatischen⁸⁷Sr/⁸⁶Sr Initialverhältnis von 0.7047. Diese Daten machen eine große Beteiligung von Mantelmaterial wahrscheinlich. Am ehesten entstanden die leukokraten Tieftal-Gneise durch magmatische Fraktionierungsprozesse aus den Ausgangsgesteinen der begleitenden tholeiitischen Metabasite. Die noch primitivere isotopische Zusammensetzung der Metabasite im Ötztalkristallin und spätarchaische/frühproterozoische sowie kambrische Komponenten in den Zirkonen der leukokraten Tieftal-Gneise weisen aber auch auf die Beteiligung alten krustalen Materials hin. Der Anteil der krustalen Komponente liegt im Bereich von 10 bis 40%. Der Tieftal-Orthogneiskörper und die begleitenden Metabasite werden als Relikte magmatischer Gesteine, die während eines frühordovizischen Riftings und der beginnenden Bildung neuer ozeanischer Kruste entstanden sind, gedeutet. Zeugen dieses Vorganges sind in allen variszisch und alpidisch geprägten Gebieten Westund Mitteleuropas zu finden.

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With 13 Figures     

The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations

We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. This revised version was published online in August 2006 with corrections to the Cover Date.     

BN objects — A class of very young and massive stars

The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object.Paper presented at a Workshop on The Role of Dust in Dense Regions of Interstellar Matter, held at Georgenthal, G.D.R., in March, 1986.     

Mass and particle ‘loading’ in plasma-neutral gas interaction

Qualitative considerations of mass and particle loading in plasma-neutral gas interaction are made by the help of a one-dimensional steady model. In the case of particle loading the plasma flow behind a strong shock is accelerated as in the case of mass loading regarded by Biermannet al. (1967) whereas behind a weak shock the flow is decelerated. As an example, one-dimensional time-dependent flows with ionization of the neutral gas by Alfvén's critical velocity effect are calculated. Because of the acceleration of the subsonic flow by loading processes, the existence of a tangential discontinuity in the flow around comets seems questionable.