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  • Cambridge University Press (CUP)  (5)
  • 2005-2009  (5)
  • 1
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2009
    In:  Journal of the Marine Biological Association of the United Kingdom Vol. 89, No. 5 ( 2009-08), p. 1083-1090
    In: Journal of the Marine Biological Association of the United Kingdom, Cambridge University Press (CUP), Vol. 89, No. 5 ( 2009-08), p. 1083-1090
    Abstract: This study reviews and updates information on cetacean strandings in the state of Ceará, Brazil (02°30′S 41°15′W– 04°30′S 36°45′W), comprising 573 km of coastline. In the years 1992–2005, there were 252 cetacean stranding events, representing 19 species: three species of Balaenopteridae, three Physeteridae, two Kogiidae, two Ziphiidae and 11 Delphinidae. Three species comprised the majority (78.9%) of stranding events: estuarine dolphin, Sotalia guianensis (61.9%); sperm whale, Physeter macrocephalus (10.3%); and rough-toothed dolphin, Steno bredanensis (6.7%). There was an increasing trend in the number of cases reported in the first five years with a highest frequency achieved in 1996. Stranding events occurred throughout the year, with the lowest frequency occurring in the autumn (March–May). Approximately 4% of the events were attributed to natural causes while 24.6% were human-related, mainly incidental captures. Meat removal for human consumption or bait was recorded in 6.7% of events. In the study area, Sotalia guianensis , P. macrocephalus and Steno bredanensis were the most abundant cetacean species, whereas Lagenodelphis hosei , Pseudorca crassidens , Orcinus orca , Kogia sima , Mesoplodon europaeus , Balaenoptera acutorostrata and Balaenoptera bonaerensis are probably rare in the area.
    Type of Medium: Online Resource
    ISSN: 0025-3154 , 1469-7769
    RVK:
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2009
    detail.hit.zdb_id: 1491269-7
    detail.hit.zdb_id: 281325-7
    SSG: 12
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  • 2
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2008
    In:  Proceedings of the International Astronomical Union Vol. 4, No. S259 ( 2008-11), p. 53-60
    In: Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 4, No. S259 ( 2008-11), p. 53-60
    Abstract: This work reports high resolution SMA polarimetric observations toward NGC 2024 FIR 5, a magnetized core previously found to harbour protostars. Our 345 GHz data indicates the presence of an extended dust emission associated with the dense core where the protostars are embedded. The 3σ polarized intensity shows depolarization toward the peak of Stokes I emission. This diminishing polarized flux implies that the alignment efficiency of the core dust grains is low within higher column densities where grain properties are likely different. The derived magnetic field geometry exhibits pinched field lines which are typical in evolved supercritical clouds where the magnetic field no longer support the core from collapsing. As a consequence for protostars, the gravitational pulling along the disk's long axis makes an equatorial bend to the field lines that, in turn, results in a hourglass shape. The SMA field structure agrees perfectly with the BIMA map. However, models are still necessary to provide a complete description of the evolutionary scenario of FIR 5.
    Type of Medium: Online Resource
    ISSN: 1743-9213 , 1743-9221
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2008
    detail.hit.zdb_id: 2170724-8
    SSG: 16,12
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  • 3
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2008
    In:  Proceedings of the International Astronomical Union Vol. 4, No. S259 ( 2008-11), p. 101-102
    In: Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 4, No. S259 ( 2008-11), p. 101-102
    Abstract: Magnetic fields are supposed to play an important role in the formation and support of self-gravitating clouds and the formation and evolution of protostars in such clouds. We used R -band linear polarimetry collected for about 12000 stars in 46 fields with lines of sight toward the Pipe nebula to investigate the properties of the magnetic fields acting on this dark cloud complex.
    Type of Medium: Online Resource
    ISSN: 1743-9213 , 1743-9221
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2008
    detail.hit.zdb_id: 2170724-8
    SSG: 16,12
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  • 4
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2009
    In:  Proceedings of the Edinburgh Mathematical Society Vol. 52, No. 1 ( 2009-02), p. 1-21
    In: Proceedings of the Edinburgh Mathematical Society, Cambridge University Press (CUP), Vol. 52, No. 1 ( 2009-02), p. 1-21
    Abstract: Using variational methods, we establish the existence and multiplicity of positive solutions for the following class of problems: where λ,β∈(0,∞), q ∈(1,2*−1), 2*=2 N /( N −2), N ≥3, V,Z :ℝ N →ℝ are continuous functions verifying some hypotheses.
    Type of Medium: Online Resource
    ISSN: 0013-0915 , 1464-3839
    RVK:
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2009
    detail.hit.zdb_id: 1465484-2
    SSG: 17,1
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  • 5
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2009
    In:  Glasgow Mathematical Journal Vol. 51, No. 2 ( 2009-05), p. 367-383
    In: Glasgow Mathematical Journal, Cambridge University Press (CUP), Vol. 51, No. 2 ( 2009-05), p. 367-383
    Abstract: In this paper we show existence of positive solutions for a class of quasi-linear problems with Neumann boundary conditions defined in a half-space and involving the critical exponent.
    Type of Medium: Online Resource
    ISSN: 0017-0895 , 1469-509X
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2009
    detail.hit.zdb_id: 1465410-6
    SSG: 17,1
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