History of the inductive sciences : from the earliest to the present time / by William Whewell.

v. 2

A history of the first half-century of the National Academy of Sciences, 1863-1913.

1863-1913

A history of the first half-century of the National Academy of Sciences, 1863-1913.

1863-1913

History of the inductive sciences : from the earliest to the present time / by William Whewell.

v.1

Building a retrospective collection in pharmacy: a brief history of the literature with some considerations for U.S. health sciences library professionals

This paper argues that historical works in pharmacy are important tools for the clinician as well as the historian. With this as its operative premise, delineating the tripartite aspects of pharmacy as a business enterprise, a science, and a profession provides a conceptual framework for primary and secondary resource collecting. A brief history and guide to those materials most essential to a historical collection in pharmacy follows. Issues such as availability and cost are discussed and summarized in checklist form. In addition, a glossary of important terms is provided as well as a list of all the major U.S. dispensatories and their various editions. This paper is intended to serve as a resource for those interested in collecting historical materials in pharmacy and pharmaco-therapeutics as well as provide a history that gives context to these classics in the field. This should provide a rationale for selective retrospective collection development in pharmacy.

Encyclopaedia Britannica : Supplement to the 4th, 5th, and 6th editions ... With preliminary dissertations on the history of the sciences ...

Supplments numbered v. 21-26 on backs.

History of the inductive sciences, from the earliest to the present times.

Mode of access: Internet.

An historical, geographical, and philosophical view of the Chinese empire; comprehending a description of the fifteen provinces of China, Chinese Tartary, tributary states; natural history of China; government, religion, laws, manners and customs, literature, arts, sciences, manufactures, &c.

Mode of access: Internet.

The ancient history of the Egyptians, Carthaginians, Assyrians, Babylonians, Medes and Persians, Grecians, and Macedonians : including a History of the arts and sciences of the ancients /

Added t.-p., engr.

A new history of the life and reign of the Czar Peter the Great, Emperor of all Russia, and father of his country : Giving an exact relation of I. His travels, studies, and personal fatigues, for the attaining of knowledge in civil and military affairs, and the improvement of his subjects. II. His introduction of arts and sciences, a naval force, and commerce with foreign nations; also his many reformations in church and state, the army, and the customs and manners of his people. III. His wars with the Swedes, Turks, Tartars and Persians; victories by sea and land; acquisitions of territory, and increase of power. IV. His regard to genius and merit, particularly in the instances of General Le Fort, Prince Menzikoff, and the Empress Catharine: and his severe justice on offenders, exemplified in the proceedings against the czarewitz, and others. /

By John Bancks.

History of the inductive sciences from the earliest to the present time.

Includes supplement.

History of the philosophy of mind: embracing the opinions of all writers on mental sciences from the earliest period to the present time.

Mode of access: Internet.

Star formation history of Canis Major R1 I. Wide-Field X-ray study of the young stellar population

Aims. The CMa R1 star-forming region contains several compact clusters as well as many young early-B stars. It is associated with a well-known bright rimmed nebula, the nature of which is unclear (fossil HII region or supernova remnant). To help elucidate the nature of the nebula, our goal was to reconstruct the star-formation history of the CMa R1 region, including the previously unknown older, fainter low-mass stellar population, using X-rays. Methods. We analyzed images obtained with the ROSAT satellite, covering similar to 5 sq. deg. Complementary VRI photometry was performed with the Gemini South telescope. Colour-magnitude and colour-colour diagrams were used in conjunction with pre-main sequence evolutionary tracks to derive the masses and ages of the X-ray sources. Results. The ROSAT images show two distinct clusters. One is associated with the known optical clusters near Z CMa, to which similar to 40 members are added. The other, which we name the ""GU CMa"" cluster, is new, and contains similar to 60 members. The ROSAT sources are young stars with masses down to M(star) similar to 0.5 M(circle dot), and ages up to 10 Myr. The mass functions of the two clusters are similar, but the GU CMa cluster is older than the cluster around Z CMa by at least a few Myr. Also, the GU CMa cluster is away from any molecular cloud, implying that star formation must have ceased; on the contrary (as already known), star formation is very active in the Z CMa region.