WR 7a: a V Sagittae or a qWR star?     

A. S. Oliveira  J. E. Steiner  D. Cieslinski 《Monthly notices of the Royal Astronomical Society》2003,346(3):963-967

The star WR 7a, also known as SPH 2, has a spectrum that resembles that of V Sagittae stars although no O  vi emission has been reported. The Temporal Variance Spectrum – TVS – analysis of our data shows weak but strongly variable emission of O  vi lines which is below the noise level in the intensity spectrum.
Contrary to what is seen in V Sagittae stars, optical photometric monitoring shows very little, if any, flickering. We found evidence of periodic variability. The most likely photometric period is   P _phot= 0.227(±14) d  , while radial velocities suggest a period of   P _spec= 0.204(±13) d  . One-day aliases of these periods can not be ruled out. We call attention to similarities with HD 45166 and DI Cru (= WR 46), where multiple periods are present. They may be associated to the binary motion or to non-radial oscillations.
In contrast to a previous conclusion by Pereira et al., we show that WR 7a contains hydrogen. The spectrum of the primary star seems to be detectable as the N  v 4604 Å  absorption line is visible. If so, it means that the wind is optically thin in the continuum and that it is likely to be a helium main sequence star.
Given the similarity to HD 45166, we suggests that WR 7a may be a qWR – quasi Wolf–Rayet – star. Its classification is WN4h/CE in the Smith, Shara & Moffat three-dimensional classification system.  相似文献   

The value of lunar material accessible for detailed studies     

Urs Krhenbühl 《Meteoritics & planetary science》2001,36(10):1292-1294

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XMM–Newton spectral properties of the narrow-line Seyfert 1 galaxy IRAS 13224 – 3809     

Th. Boller  Y. Tanaka  A. Fabian  W. N. Brandt  L. Gallo  N. Anabuki  Y. Haba  S. Vaughan 《Monthly notices of the Royal Astronomical Society》2003,343(4):L89-L93

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The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM–Newton deep fields     

M. A. Worsley  A. C. Fabian  F. E. Bauer  D. M. Alexander  G. Hasinger  S. Mateos  H. Brunner  W. N. Brandt  D. P. Schneider 《Monthly notices of the Royal Astronomical Society》2005,357(4):1281-1287

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Solar Physics at the Goddard Space Flight Center     

John C. Brandt 《Solar physics》1969,6(3):490-497

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Some General Properties of Transverse Motions of the Geostrophic Front     

Dotsenko  S. F.  Rubino  A.  Brandt  P. 《Physical Oceanography》2003,13(4):189-200

Within the framework of the reduced-gravity model of the ocean taking into account the effect of friction in the Rayleigh form, we study the two-dimensional problem of nonlinear motions of a subsurface front of finite width. We consider the conservation laws and the character of motion of the center-of-mass of the cross section of the front and their variations caused by the losses of energy. For fields with special structure, the problem is reduced to the solution of a system of nonlinear ordinary differential equations. It is shown that the initially geostrophic frontal current decays with time according to a power law. The deviations of the initial state of the front from the state of geostrophic balance result in the generation of superinertial oscillations of the hydrodynamic fields.  相似文献   

Illite crystallinity patterns in the Anti-Atlas of Morocco     

Geoffrey M. H. Ruiz  Urs Helg  François Negro  Thierry Adatte  Martin Burkhard 《Swiss Journal of Geoscience》2008,101(2):387-395

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Earthquakes in Switzerland and surrounding regions during 2007     

Nicolas Deichmann  Manfred Baer  John Clinton  Stephan Husen  Donat Fäh  Domenico Giardini  Philipp Kästli  Urs Kradolfer  Stefan Wiemer 《Swiss Journal of Geoscience》2008,101(3):659-667

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Indigenous resource management and external development interventions in the Dry Zone of Sri Lanka: From conflicts to synergies?     

Geiser Urs 《GeoJournal》1995,35(2):185-196

An argument is presented that environmental problems in the Dry Zone of Sri Lanka are caused, among other reasons, by conflicts between the exogenously influenced modern strategy of land resources management, and the incompatibility of the modern approach with aspects of the physical environment. This conclusion is obtained through a comparative analysis of both strategies using an actor-oriented methodology. Concerning the potential of indigenous technologies under present-day conditions it is argued that the rationale guiding them is highly relevant and has actually been internalized into the vocabulary of many development interventionists because negative effects of the dominant development discourse are becoming obvious. A shift in power relations (including the acceptance of local knowledge within innovative development ventures) is required if the potential of the indigenous strategy is to be tapped. It remains an open question whether this power shift can take place from within the development enterprise alone.Many thanks to Jayantha Perera, Heidi Stutz and Ben Wisner for critical comments on a first draft of this paper.  相似文献   

The age and source of late Hercynian magmatism in the central Alps: evidence from precise U−Pb ages and initial Hf isotopes   总被引：1，自引：0，他引：1  

Urs Schaltegger  Fernando Corfu 《Contributions to Mineralogy and Petrology》1992,111(3):329-344

This study presents U–Pb ages for zircon, titanite, allanite and epidote, and initial Hf isotopic compositions for zircon of Upper Carboniferous granites, diorites and syenites from the Aar massif, central Alps. The rocks were emplaced during three magmatic pulses after Hercynian collisional tectonics: (A) a shoshonitic-ultrapotassic series at 334±2.5 Ma; (B) scattered diorites and granites at 308–310 Ma; and (C) a high-K cale-alkaline granite batholith at 298±2 Ma. Inheritance of old zircons is negligible among all three groups. The Southern Aar granite, in contrast, is a syn-tectonic, probably ca. 350 Ma old granite that contains large amounts of inherited Precambrian zircons. Alpine metamorphism caused weak lead loss in many analyzed zircon fractions, but left the titanite U–Pb system undisturbed: thorites were almost completely reset by Alpine and recent lead loss. Mineral isochrons defined by titanite, allanite, epidote and apatite yield initial Pb isotopic compositions that are in agreement with the model values of Stacey and Kramers. Initial Hf isotopic compositions range from _Hf=–8 to +3.5. The data follow a trend of increasing _Hf with decreasing age. The _Hf versus element concentration relationships suggest mixing between a mantle and a crustal component. These relationships can be explained in terms of generation of the melts from a subcontinental mantle that had been enriched during subduction events at about 1 Ga and by 300 Ma had developed an isotopic signature distinct from that of MORB-type mantle. Further contamination of the melts occurred during ascent and differentiation in the crust. This late Hercynian magmatism can be related to post-collisional strike-slip tectonics.  相似文献