13/5/20, [football] association, Saint-Ouen, équipe du Red Star club : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59263

13/5/20, [football] association, Saint-Ouen, équipe du Red Star club : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59264

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, Red Star contre R.C.F. [Racing Club de France] : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59140

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, Red Star contre R.C.F. [Racing Club de France] : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59141

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, Red Star contre R.C.F. [Racing Club de France] : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59143

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, Red Star contre R.C.F. [Racing Club de France] : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59144

7/3/20, Stade Bergeyre, [football] association, équipe du Red Star : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 58360

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, équipe [du] Red Star : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59147

2/5/20, [stade Bergeyre], championnat de Paris, [football] association, équipe [du] Red Star : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59148

Red Star, stade Bergeyre, 23/5/20 [équipe de football] : [photographie de presse] / [Agence Rol]

Référence bibliographique : Rol, 59386

Red Star on military affairs, 1945-1952 ; a selected, annotated list of articles in the Soviet military newspaper /

U.S. Air Force Project Rand.

The Corio Oval Tribe : a prosopographical perspective of the Geelong Football Club in the nineteenth century

This article analyses the occupational and class status of Geelong footballers in the nineteenth century via the methodology of prosopography. Prosopography is an empirical group biography approach to historical research. The article argues that during the period 1859-78 Geelong's playing group was largely derived from the squattocracy and urban middle class. In the later period 1878-96 the Geelong club recruited more widely from the working class, as in keeping with the increased participation of this class in football from the late 1870s. It can be argued that this more diverse group helped establish Geelong as a footballing power.

The Amplifier - v. 2, no. 14

In this issue...Dean Adami, M club, Red Rock, Bernice, Montana, Mineral Club, Mines Football, Sam Worcester, Professor Laity, Western Civilization class

Infared observations of H II regions

Spectral data are presented, giving intensities of the Brackett ɤ (B₇) line at six positions in M 42 and of the Brackett ten through fourteen (B₁₀-B₁₄) lines plus the He 4d³D-3p³p⁰ line at three positions in M 42. Observations of the Brackett ɤ line are also given for the planetary nebulae NGC 7027 and IC 418. Brackett gamma is shown to exhibit an anomalous satellite line in NGC 7027. Broadband data are presented, giving intensities at effective wavelengths of 1.25 μ, 1.65 μ, 2.2 μ, 3.5 μ and 4.8 μ for three positions in M 42.

Comparisons with visual and radio data as well as 12 micron and 20 micron data are used to derive reddening, electron temperatures, and electron densities for M 42 and the two planetaries, as well as a helium abundance for M 42. A representative electron temperature of 8400°K ± 1000°K, an electron density of 1.5 ±0.1 x 10³ cm^-3 and a He/H number density ratio of 0.10 +0.10/-0.05 are derived for the central region of M 42. The electron temperature is found to increase slightly with distance from the Trapezium.

M 42 is shown to emit in excess of the predicted recombination radiation throughout the entire infrared spectrum. The variations in the excess with wavelength and with position are analyzed to determine which of several physical processes may be operating. The longer wavelength infrared excess is shown to be dominated by dust emission, while the shorter wavelength infrared excess is caused by dust scattering. The dust is shown to be larger than the average interstellar particle. A new feature of the Orion red star ORS-1 is found in that it appears to have a reflection nebula around it.