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  • 1
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Physics of the Earth and Planetary Interiors 31 (1983), S. 277-280 
    ISSN: 0031-9201
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 69 (1980), S. 94-106 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Abstract Muscovites in metapelites belonging to the Chloritoid, Staurolite, Kyanite, Sillimanite-K feldspar and Sillimanite-K feldspar-Cordierite zones of the Sierra de Guadarrama metamorphic area, have a chemical composition close to the end member Ms (mean value around Ms 92); nevertheless, they show definite variations in Al2O3, K2O and Na2O contents and, to a lesser extent, in FeO and MgO. These chemical variations (i. e., a progressive decrease of celadonite content, a increase followed by a decrease in paragonite solid solution towards compositions close to the endmember muscovite) may be regarded as in a close relationship with metamorphic grade in the upper metamorphic zones (Chloritoid, Staurolite and Kyanite zones), but the corresponding variations in the remaining lower zones (that is, a slight increase in Fe and Mg coupled with a slight increase in AlVI and Ti, and more or less abrupt changes in Na and K contents) can only be explained considering the interference of anatectic phenomena, which modificate the normal trends due to changes in metamorphic grade. As a consequence of these observations, it has been concluded that muscovite composition in metapelites can only be used as an indicator of metamorphic grade in conditions where partial melting phenomena are absent.
    Abstract: Résumé Les muscovites des métapélites de la Sierra de Guadarrama, appartenant aux zones à chloritoïde, staurotide, disthène, sillimanite-feldspath potassique et sillimanite-feldspath potassique-cordierite, ont une composition chimique très proche de la valeur theorique (valeur moyenne Ms 92); néanmoins elles présentent une certaine variation dans les teneurs en Al2O3, K2O et Na2O et, à une moindre échelle, en FeO et MgO. Ces variations chimiques (diminution progressive en céladonite, augmentation suivie d'une diminution de la paragonite vers des compositions proches de la muscovite sensu stricto) que présentent les muscovites des zones à chloritoïde, staurotide et disthène sont étroitement liées aux zones métamorphiques superieures. Au contraire, les variations (legère augmentation des teneurs en Fe et Mg, legère diminution en AlVI et Ti, et plus ou moins brusques variations en Na et K, respectivement) correspondantes des muscovites des zones de la sillimanite-feldspath potassique et de la sillimanite-feldspath potassiquecordiérite, ne peuvent s'expliquer que si l'on admis que, dans les niveaux plus métamorphiques, les muscovites souffrent une série de changements chimiques dûs au début de l'anatexie, laquelle modifie les tendances normales liées à l'intensité du metamorphisme. En conséquence, seules les muscovites des métapélites situées au-dessus de l'isograde du feldspath potassique, en dehors de toute fusion partielle peuvent être utilisées pour déterminer le degré de métamorphisme des roches qui les contiennent.
    Notes: Zusammenfassung Muskovite in Metapeliten, die zu den Chloritoid, Staurolit, Cyanit, Sillimanit-K-Feldspat und Sillimanit-K-Feldspat-Cordierit Zonen der Sierra Guadarrama Metamorphgebiet gehören, zeigen einen Chemismus, der sich dem Endglied Muskovit nähert (Durchschnitt etwa Ms 92). Es wurden trotzdem bestimmte Veränderungen in den Gehalten von hauptsächlich Al2O3, K2O und Na2O und in geringerem Ausmaß in FeO und MgO festgestellt. Diese chemischen Veränderungen (d. h. ein progressives Abnehmen des Keladonitgehaltes, gefolgt von einer Abnahme der Paragonitmischungsreihe in einer Richtung, die sich dem Endglied Muskovit annähert) können in einem engen Zusammenhang mit der höher metamorphen Zone (Chloritoid-, Staurolit- und Cyanitzonen) gesehen werden. Die entsprechenden Veränderungen in den tieferen Zonen (d. h. eine minimale Abnahme von Fe und Mg begleitet von einer ebenfalls geringen Abnahme von Al und Ti und einer mehr oder weniger abrupten Veränderung im Na- und K-Gehalt) können jedoch nur unter Berücksichtigung der Interferenz von anatektischen Phänomenen gesehen werden. Solche Phänomene modifizieren den normalen Trend durch eine Veränderung des Metamorphosegrades. Daraus folgt, daß die Muskovitzusammensetzung als Indikator des Metamorphosegrades nur in Abwesenheit von partiellen Schmelzphenomen gebraucht werden kann.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 169 (1990), S. 37-39 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We present preliminary results of CCD BV photometry of the old open cluster King 2. The values obtained for the main parameters are:E(B-V)=0.31, (m-M)0=13.78, metal content approximately solar, and age 6×109 yr. From the comparison with synthetic colour-mgnitude diagrams generated by models with overshoot we try to answer the question whether or not convective elements generated in the core can penetrate into the surrounding stable zone (separated by a discontinuity of molecular weight).
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Plant systematics and evolution 184 (1993), S. 11-25 
    ISSN: 1615-6110
    Keywords: Cistaceae ; Tuberaria ; Karyology ; hybridization ; backcrossing ; polyploidy ; autogamy ; Flora of S Spain
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract A polyploid complex ofTuberaria sect.Scorpioides species in S Spain has been studied. We have found the chromosome numbers n = 12 and 18, which probably originated from the extinct base number x = 6 by means of allopolyploidy. Octoploids (n = 24) seem to be the result of different crossings, and fall morphologically withinT. guttata, T. inconspicua, orT. commutata. Backcrosses between octoploids and tetraploids originate new hexaploids (n = 18), which, once stabilized, behave as amphidiploids. Most of these also fall within the traditional concept ofT. guttata, so that the enormous polymorphism of this taxon seems to be justified.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Experimental mechanics 38 (1998), S. 24-28 
    ISSN: 1741-2765
    Keywords: Cable-stayed bridge ; bridge monitoring ; segmental construction ; instrumentation ; model updating ; vibration testing
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Notes: Abstract The Alamillo Bridge is one of the long-span bridges crossing the Guadalquivir River. It was built on the occasion of Expo '92 in 1992 in Sevilla, Spain. The bridge is a cable-stayed structure spanning 200 m without any intermediate supports. Its originality is the lack of back stays and the balancing of the front stays through the backward inclination of a massive pylon. This paper shows the importance of experimental in situ techniques when applied to unconventional civil engineering structures and how—with the help of an important amount of accurate instrumentation, monitoring the most important experimental variables—it was possible to build the bridge correctly, safely, and on schedule.
    Type of Medium: Electronic Resource
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  • 6
    Publication Date: 2016-06-06
    Print ISSN: 0038-0938
    Electronic ISSN: 1573-093X
    Topics: Physics
    Published by Springer
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  • 7
    Publication Date: 2015-08-20
    Description: We present a method to identify ultrafaint dwarf galaxies (UFDGs) candidates in the halo of the Milky Way using the future Gaia catalogue and we explore its detection limits and completeness. The method is based on the Wavelet Transform and searches for overdensities in the combined space of sky coordinates and proper motions, using kinematics in the search for the first time. We test the method with a Gaia mock catalogue that has the Gaia Universe Model Snapshot as a background, and use a library of around 30 000 UFDGs simulated as Plummer spheres with a single stellar population. For the UFDGs, we use a wide range of structural and orbital parameters that go beyond the range spanned by real systems, where some UFDGs may remain undetected. We characterize the detection limits as function of the number of observable stars by Gaia in the UFDGs with respect to that of the background and their apparent sizes in the sky and proper motion planes. We find that the addition of proper motions in the search improves considerably the detections compared to a photometric survey at the same magnitude limit. Our experiments suggest that Gaia will be able to detect UFDGs that are similar to some of the known UFDGs even if the limit of Gaia is around 2 mag brighter than that of SDSS, with the advantage of having a full-sky catalogue. We also see that Gaia could even find some UFDGs that have lower surface brightness than the SDSS limit.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 8
    Publication Date: 2015-05-30
    Description: In this paper, we combine Wide Field Camera3/UVIS F 275 W , F 336 W , and F 438 W data from the ‘UV Legacy Survey of Galactic Globular Clusters: Shedding Light on Their Populations and Formation’ (GO 13297) Hubble Space Telescope Treasury programme with F 606 W , F 625 W , F 658 N , and F 814 W Advanced Camera for Surveys archive data for a multiwavelength study of the globular cluster NGC 6352. In the colour–magnitude and two-colour diagrams obtained with appropriate combination of the photometry in the different bands, we separate two distinct stellar populations and trace them from the main sequence to the subgiant, red giant, horizontal and asymptotic giant branches. We infer that the two populations differ in He by Y  = 0.029 ± 0.006. With a new method, we also estimate the age difference between the two sequences. Assuming no difference in [Fe/H] and [α/Fe], and the uncertainties on Y , we found a difference in age between the two populations of 10 ± 120 Myr. If we assume [Fe/H] and [α/Fe] differences of 0.02 dex (well within the uncertainties of spectroscopic measurements), the total uncertainty in the relative age rises to ~300 Myr.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 9
    Publication Date: 2016-04-04
    Description: Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. However, the lack of a large number of OCs analysed homogeneously hampers the investigations about chemical patterns and the existence of Galactocentric radial and vertical gradients, or an age–metallicity relation. To overcome this, we have designed the Open Cluster Chemical Abundances from Spanish Observatories (OCCASO) survey. We aim to provide homogeneous radial velocities, physical parameters and individual chemical abundances of six or more red clump stars for a sample of 25 old and intermediate-age OCs visible from the Northern hemisphere. To do so, we use high-resolution spectroscopic facilities ( R ≥ 62 000) available at Spanish observatories. We present the motivation, design and current status of the survey, together with the first data release of radial velocities for 77 stars in 12 OCs, which represents about 50 per cent of the survey. We include clusters never studied with high-resolution spectroscopy before (NGC 1907, NGC 6991, NGC 7762), and clusters in common with other large spectroscopic surveys like the Gaia -ESO Survey (NGC 6705) and Apache Point Observatory Galactic Evolution Experiment (NGC 2682 and NGC 6819). We perform internal comparisons between instruments to evaluate and correct internal systematics of the results, and compare our radial velocities with previous determinations in the literature, when available. Finally, radial velocities for each cluster are used to perform a preliminary kinematic study in relation with the Galactic disc.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 10
    Publication Date: 2016-06-17
    Description: We report the discovery of an optical Einstein ring in the Sculptor constellation, IAC J010127-334319, in the vicinity of the Sculptor dwarf spheroidal galaxy. It is an almost complete ring (~300°) with a diameter of ~4.5 arcsec. The discovery was made serendipitously from inspecting Dark Energy Camera (DECam) archive imaging data. Confirmation of the object nature has been obtained by deriving spectroscopic redshifts for both components, lens and source, from observations at the 10.4 m Gran Telescopio CANARIAS (GTC) with the spectrograph OSIRIS. The lens, a massive early-type galaxy, has a redshift of z  = 0.581, while the source is a starburst galaxy with redshift of z  = 1.165. The total enclosed mass that produces the lensing effect has been estimated to be M tot  = (1.86 ± 0.23) x 10 12 M .
    Print ISSN: 1745-3925
    Electronic ISSN: 1745-3933
    Topics: Physics
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