Poetae minores graeci.

v. 1. Hesiodi carmina.--v. 2. Scholia ad Hesiodum e codd. mss.--v. 3. Theognidis, Archilochi, Solonis, Simonidis, Tyrtaei, Empedoclis, Parmenidis, Sapphonis, Alcaei, Stesichori et aliorum fragmenta.-v. 4. Theocriti, Bionis et Moschi Carmina bucolica ex recensione L.C. Valckenarii.--v. 5. Scholia ad Theocritum e codd. mss.

Suidae lexicon : graece et latine /

Preface by Ludolf Küster.

Herodoti Historiarum libri IX.

Greek title at head of title-page.

Georgii Choerobosci Dictata in Theodosii Canones, necon Epimerismi in psalmos.

Mode of access: Internet.

Principles of the Reformation. A sermon preached November 16, 1826, at the dedication of the house of public worship of the First Congregational Society in Salem. ...

Appendix, pp.[50]-62, contains a "Brief historical sketch of the First Church in Salem," with an illustration of the meeting-house built in 1718.

Hēphaistiōnos Encheiridion peri metrōn kai poiēmatōn = Hephaestionis Alexandrini Enchiridion /

Includes bibliographical references and indexes.

Museé de peinture et de sculpture, ou, Recueil des principaux tableaux, statues et bas-reliefs des collections publiques et particulières de l'Europe /

Vol. 16 has title: Les loges du Vatican, sujets peints a ̀fresque, par Raphael.

[Album de vues et de monuments de Venise et de Rome] / [photogr. par Antonio Perini et Giacomo Caneva]

Ancien possesseur : Rothschild, Adèle de (1843-1922)

Uber Kartenprojection. Abhandlungen von Lagrange (1779) und Gauss (1822)

Mode of access: Internet.

Minutes of the right worshipful Grand lodge of the most ancient nad honorable fraternity of Free and accepted masons of Pennsylvania and masonic jurisdiction thereunto belonging. v. 1-12: 1779 to 1880.

Vols. 1-6 compiled by Joshua L. Lyte.

On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09

e argue that the extraordinary fact that all three known millisecond pulsars are very close to the galactic plane implies that there must be ~100 potentially observable millisecond pulsars within ~4 kpc from the Sun. Our other main conclusion is that the dipole magnetic fields or old neutron stars probably saturate around 5 x 108 gauss.

Direct and Inverse Scattering for Beltrami Fields

We consider an obstacle scattering problem for linear Beltrami fields. A vector field is a linear Beltrami field if the curl of the field is a constant times itself. We study the obstacles that are of Neumann type, that is, the normal component of the total field vanishes on the boundary of the obstacle. We prove the unique solvability for the corresponding exterior boundary value problem, in other words, the direct obstacle scattering model. For the inverse obstacle scattering problem, we deduce the formulas that are needed to apply the singular sources method. The numerical examples are computed for the direct scattering problem and for the inverse scattering problem.

Direct and Inverse Scattering for Beltrami Fields

We consider an obstacle scattering problem for linear Beltrami fields. A vector field is a linear Beltrami field if the curl of the field is a constant times itself. We study the obstacles that are of Neumann type, that is, the normal component of the total field vanishes on the boundary of the obstacle. We prove the unique solvability for the corresponding exterior boundary value problem, in other words, the direct obstacle scattering model. For the inverse obstacle scattering problem, we deduce the formulas that are needed to apply the singular sources method. The numerical examples are computed for the direct scattering problem and for the inverse scattering problem.