Browsing Saint Mary's Faculty Articles and Other Works by Title

Browsing Saint Mary's Faculty Articles and Other Works by Title

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  • Bullerwell, Wendy L.; MacGillivray, Leonard R.; Zaworotko, Michael J.; Vaughan, Keith, 1943-; Wilman, Derry E. V. (Intemational Union of Crystallography, 1995)
    In the crystal structure of the title compound, 4-(3,3-dimethyl-l-triazeno)benzamide, C[subscript 9]H[subscript I2]N[subscript 4]0, (2), the N=N double bond [1.282 (8) [Angstrom]] is 0.030 [Angstrom] shorter than the N-N ...

  • Fei, Houman; McVetty, Peter B. E.; Vessey, Joseph Kevin (Elsevier, 2013-04)
    Four genotypes of B. napus (cultivars Topas, Sentry and Polo, and the experimental line 04C204) varying in seed oil content (SOC) potential (from 42.2% to 50.0% seed DW) were used to study C and N partitioning among shoots, ...

  • Gallo, Luigi C.; MacMackin, C.; Vasudevan, R.; Cackett, E. M.; Fabian, A. C.; Panessa, F. (Oxford University Press, 2013-07)

    1ES 1927+654 is an active galactic nucleus (AGN) that appears to defy the unification model. It exhibits a type-2 optical spectrum, but possesses little X-ray obscuration. XMM–Newton and Suzaku ...


  • Gallo, Luigi C.; Fabian, A. C.; Zoghbi, A.; Wilkins, D. R.; Dwelly, T.; Uttley, P.; Schartel, N.; Miniutti, G.; Grupe, D.; Komossa, S. (Oxford University Press, 2012)
    The narrow-line Seyfert 1 Galaxy 1H 0707−495 went into a low state from 2010 December to 2011 February, discovered by a monitoring campaign using the X-Ray Telescope on the Swift satellite. We triggered a 100 ks XMM–Newton ...

  • Biradha, Kumar; Zaworotko, Michael J.; Nangia, Ashwini; Desiraju, Gautam R. (International Union of Crystallography, 1997)
    In contrast to the stacking characteristic of quinones, the title compound, C[subscript 20]H[subscript 12]O[subscript 4], forms a two-dimensional network of C--H...O hydrogen bonds. The molecule has an unsymmetrical butterfly ...

  • Khan, Mahmood-ul-Hassan; Hameed, Shahid; Akhtar, Tashfeen; Masuda, Jason Douglas, 1977- (International Union of Crystallography, 2009-06)
    In the title compound, C[subscript 8]H[subscript 9]NS, the dihedral angle between the aromatic ring and the thioamide fragment is 36.0 (2)[degrees ]. There are [pi]-stacking interactions between coplanar aryl fragments, ...

  • Khan, Mahmood-ul-Hassan; Hameed, Shahid; Akhtar, Tashfeen; Masuda, Jason Douglas, 1977- (International Union of Crystallography, 2009)
    The title compound, C[subscript 7]H[subscript 6]BrNS, crystallizes with two molecules in the asymmetric unit. The dihedral angles between the aromatic ring and the thioamide fragment are 23.6 (4) and 20.5 (3)[degrees] in ...

  • Khan, Mahmood-ul-Hassan; Hameed, Shahid; Akhtar, Tashfeen; Masuda, Jason Douglas, 1977- (International Union of Crystallography, 2009)
    In the title compound, C[subscript 7]H[subscript 6]ClNS, the dihedral angle between the aromatic ring and the thioamide fragment is 28.1 (2)[degrees]. The structure features a [pi]-stacking interaction between the aromatic ...

  • Piorko, Adam; Christie, Sean; Zaworotko, Michael J. (International Union of Crystallography, 1994-10)
    The structure of [(5a,6,7,8,9,9a-[eta superscript 6])-[1,4]benzodi-oxino[2,3-b]pyridine]([eta superscript 5]-cyclopentadienyl)iron(II)hexafluorophosphate, [Fe(C[subscript 5]H[subscript 5])(C[subscript 11] H[subscript ...

  • Wiacek, A.; Martin, R. V.; Bourassa, A. E.; Lloyd, N. D.; Degenstein, D. A. (Copernicus Publications, 2013-10)

    The limb-scatter satellite viewing geometry is well suited to detecting low-concentration aerosols in the upper troposphere due to its long observation path length (∼ 200 km), high vertical resolution (∼ 1–2 ...


  • Houlihan, Ron (Emerald Group, 2005)
    Purpose – To provide theoretical and practical perspectives on the “library as space” debate as well as an update of an earlier (2002) New Library World article on one university library’s attempt tore-position itself ...

  • Wurster, James Howard; Thacker, Robert John, 1970- (Oxford University Press, 2013-05)
    A recent approach to simulating localized feedback from active galactic nuclei (AGN) by Power et al. uses an accretion disc particle to represent both the black hole and its accretion disc. We have extrapolated and adapted ...

  • Capuano, Paolo; Russo, Guido; Civetta, Lucia; Orsi, Giovanni; D’Antonio, Massimo; Moretti, Roberto (American Geophysical Union, 2013-10)
    We present an improved density model and a new structural map of the Neapolitan Yellow Tuff caldera, the active portion of the nested Campi Flegrei caldera. The model was built using a new 3-D inversion of the available ...

  • Hambleton, K. M.; Gibson, Brad K.; Brook, C. B.; Stinson, G. S.; Conselice, C. J.; Bailin, J.; Couchman, H.; Wadsley, J. (Royal Astronomical SocietyOxford University Press, 2011)
    Encoded within the morphological structure of galaxies are clues related to their formation and evolutionary history. Recent advances pertaining to the statistics of galaxy morphology include sophisticated measures of ...

  • MacKinnon, John E. (John Hopkins University Press, 1996)
    There is no abstract available for this article.

  • Guenther, David B.; Dinescu, Dana I.; Demarque, Pierre; Pinsonneault, M. H. (American Astronomical Society, 1995-05)
    Theoretical isochrones have been constructed using the OPAL opacities to derive the ages of the open clusters NGC 188, M67, and NGC 752 as well as to estimate the amount of convective overshoot at the convective core edge. ...

  • Turner, David Gerald, 1945-; Majaess, Daniel J.; Lane, D. J.; Balam, D. D.; Gieren, W. P.; Storm, J.; Forbes, D. W.; Havlen, R. J.; Alessi, B. (Oxford Academic, 2012-05)
    The parameters for the newly discovered open cluster Alessi 95 are established on the basis of available photometric and spectroscopic data, in conjunction with new observations. Colour excesses for spectroscopically ...

  • Fuller, Todd M.; West, Michael J.; Bridges, Terry J. (American Astronomical SocietyIOP Science, 1999-07-01)
    We have examined the orientations of brightest cluster galaxies (BCGs) in poor MKW (Morgan, Kayser, and White) and AWM (Albert, White, and Morgan) clusters and find that, like their counterparts in richer Abell clusters, ...

  • Recchi, S.; Calura, F.; Gibson, Brad K.; Kroupa, P. (Oxford University Press, 2014-01)
    The aim of this paper is to quantify the amplitude of the predicted plateau in [α/Fe] ratios associated with the most metal-poor stars of a galaxy. We assume that the initial mass function (IMF) in galaxies is steeper ...

  • Guenther, David B.; Demarque, P. (American Astronomical Society, 2000-03)
    Detailed models of [alpha] Centauri A and B based on the Hipparcos, Yale, and Soderhjelm parallaxes are compared. The consequences of the uncertainty in mass, luminosity, surface temperature, and composition on the structure ...