Dissertacion Historica I : que excluye la existencia de monges Basilios en el antiguo Venerable Santuario de el Santo Sepulcro de Valencia contra las noticias falsas ... del Dr. Agustín Sales, en el cap. IV de las Memorias del mismo Santo Sepulcro

Contiene: Dissertacion historica II: que demuystra aver cursado el Patriarca Santo Domingo los estudios de artes, y de theologia en la ciudad de Palencia ... Obispado, y escritos de Idacio Galiciano el Historico ...

Manifiesto que presenta la ciudad de Valencia del servicio hecho a S. M. por si y demas pueblos de sus Gobernaciones durante la guerra con la Francia, de la gente que ha suministrado para el real servicio ... donativos y demas ..

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Dissertacion Historica I : que excluye la existencia de monges Basilios en el antiguo Venerable Santuario de el Santo Sepulcro de Valencia contra las noticias falsas ... del Dr. Agustín Sales, en el Cap. IV de las Memorias del mismo Santo Sepulcro

Contiene : Dissertacion historica II: que demuestra aver cursado el Patriarca Santo Domingo los estudios de artes, y de theologia en la ciudad de Palencia ... Obispado, y escritos de Idacio Galiciano el Historico ... ; Dissertacion III : curiosa, sobre la patria, obispado, y escritos de Idacio Galiciano el Hitorico ..

Recueil d'ouvrages curieux de mathematique et de mecanique, ou description du cabinet de monsieur Grollier de Serviere [Texto impreso] : avec des figures en taille douce

Sign.: a4, e4, i6, A-O4

Exercitia spiritualia... [Texto impreso]

Colofón

De birreto rubeo dando S.R.E. Cardinalibus Regularibus responsa... [Texto impreso]

Hoja con grab. xil. a dos tintas

Las grandezas de el restaurador de los estados de la Yglesia ... Cardenal don Gil de Albornoz, ... [Texto impreso]

Sign.: A-B2, C4, D-N2, O4, P-Z2, 2A-B2

Arte de encomendarse a Dios, o sea Virtudes de la oracion [Texto impreso]

Sign. : *-3*8, A-N8, O4

NMR characterization of lignins in Arabidopsis altered in the activity of ferulate 5-hydroxylase

Nuclear magnetic resonance (NMR) of isolated lignins from an Arabidopsis mutant deficient in ferulate 5-hydroxylase (F5H) and transgenic plants derived from the mutant by overexpressing the F5H gene has provided detailed insight into the compositional and structural differences between these lignins. Wild-type Arabidopsis has a guaiacyl-rich, syringyl-guaiacyl lignin typical of other dicots, with prominent β-aryl ether (β–O–4), phenylcoumaran (β–5), resinol (β–β), biphenyl/dibenzodioxocin (5–5), and cinnamyl alcohol end-group structures. The lignin isolated from the F5H-deficient fah1–2 mutant contained only traces of syringyl units and consequently enhanced phenylcoumaran and dibenzodioxocin levels. In fah1–2 transgenics in which the F5H gene was overexpressed under the control of the cauliflower mosaic virus 35S promoter, a guaiacyl-rich, syringyl/guaiacyl lignin similar to the wild type was produced. In contrast, the isolated lignin from the fah1–2 transgenics in which F5H expression was driven by the cinnamate 4-hydroxylase promoter was almost entirely syringyl in nature. This simple lignin contained predominantly β-aryl ether units, mainly with erythro-stereochemistry, with some resinol structures. No phenylcoumaran or dibenzodioxocin structures (which require guaiacyl units) were detectable. The overexpression of syringyl units in this transgenic resulted in a lignin with a higher syringyl content than that in any other plant we have seen reported.

Three-dimensional model of the potyviral genome-linked protein.

The full sequence of the genome-linked viral protein (VPg) cistron located in the central part of potato virus Y (common strain) genome has been identified. The VPg gene codes for a protein of 188 amino acids, with significant homology to other known potyviral VPg polypeptides. A three-dimensional model structure of VPg is proposed on the basis of similarity of hydrophobic-hydrophilic residue distribution to the sequence of malate dehydrogenase of known crystal structure. The 5' end of the viral RNA can be fitted to interact with the protein through the exposed hydroxyl group of Tyr-64, in agreement with experimental data. The complex favors stereochemically the formation of a phosphodiester bond [5'-(O4-tyrosylphospho)adenylate] typical for representatives of picornavirus-like viruses. The chemical mechanisms of viral RNA binding to VPg are discussed on the basis of the model structure of protein-RNA complex.

On the nature of the galactic early-B hypergiants

Aims. Despite their importance to a number of astrophysical fields, the lifecycles of very massive stars are still poorly defined. In order to address this shortcoming, we present a detailed quantitative study of the physical properties of four early-B hypergiants (BHGs) of spectral type B1-4 Ia+; Cyg OB2 #12, ζ1 Sco, HD 190603 and BP Cru. These are combined with an analysis of their long-term spectroscopic and photometric behaviour in order to determine their evolutionary status. Methods. Quantitative analysis of UV–radio photometric and spectroscopic datasets was undertaken with a non-LTE model atmosphere code in order to derive physical parameters for comparison with apparently closely related objects, such as B supergiants (BSGs) and luminous blue variables (LBVs), and theoretical evolutionary predictions. Results. The long-term photospheric and spectroscopic datasets compiled for the early-B HGs revealed that they are remarkably stable over long periods ( ≥ 40 yrs), with the possible exception of ζ1 Sco prior to the 20th century; in contrast to the typical excursions that characterise LBVs. Quantitative analysis of ζ1 Sco, HD 190603 and BP Cru yielded physical properties intermediate between BSGs and LBVs; we therefore suggest that BHGs are the immediate descendants and progenitors (respectively) of such stars, for initial masses in the range ~30−60 M⊙. Comparison of the properties of ζ1 Sco with the stellar population of its host cluster/association NGC 6231/Sco OB1 provides further support for such an evolutionary scenario. In contrast, while the wind properties of Cyg OB2 #12 are consistent with this hypothesis, the combination of extreme luminosity and spectroscopic mass (~110 M⊙) and comparatively low temperature means it cannot be accommodated in such a scheme. Likewise, despite its co-location with several LBVs above the Humphreys-Davidson (HD) limit, the lack of long term variability and its unevolved chemistry apparently excludes such an identification. Since such massive stars are not expected to evolve to such cool temperatures, instead traversing an O4-6Ia → O4-6Ia+ → WN7-9ha pathway, the properties of Cyg OB2 #12 are therefore difficult to understand under current evolutionary paradigms. Finally, we note that as with AG Car in its cool phase, despite exceeding the HD limit, the properties of Cyg OB2 #12 imply that it lies below the Eddington limit – thus we conclude that the HD limit does not define a region of the HR diagram inherently inimical to the presence of massive stars.

The little-studied cluster Berkeley 90 I. LS III +46 11: a very massive O3.5 If* + O3.5 If* binary

Context. It appears that most (if not all) massive stars are born in multiple systems. At the same time, the most massive binaries are hard to find owing to their low numbers throughout the Galaxy and the implied large distances and extinctions. Aims. We want to study LS III +46 11, identified in this paper as a very massive binary; another nearby massive system, LS III +46 12; and the surrounding stellar cluster, Berkeley 90. Methods. Most of the data used in this paper are multi-epoch high S/N optical spectra, although we also use Lucky Imaging and archival photometry. The spectra are reduced with dedicated pipelines and processed with our own software, such as a spectroscopic-orbit code, CHORIZOS, and MGB. Results. LS III +46 11 is identified as a new very early O-type spectroscopic binary [O3.5 If* + O3.5 If*] and LS III +46 12 as another early O-type system [O4.5 V((f))]. We measure a 97.2-day period for LS III +46 11 and derive minimum masses of 38.80 ± 0.83 M⊙ and 35.60 ± 0.77 M⊙ for its two stars. We measure the extinction to both stars, estimate the distance, search for optical companions, and study the surrounding cluster. In doing so, a variable extinction is found as well as discrepant results for the distance. We discuss possible explanations and suggest that LS III +46 12 may be a hidden binary system where the companion is currently undetected.

Somma di tutta la filosofia di Aristotele /

Mode of access: Internet.

Institutio pricipis christiani saluberrimis referta praeceptis /

Mode of access: Internet.

Claudii Fleurii ... Historia Ecclesiastica /

Mode of access: Internet.