MAUVE
发表于 2025-3-26 22:02:02
W. Wamsteker,J. J. Lorre,H. E. Schusterion, where the definition of self is affirmed through differentiation from the other. The chapter investigates how correctional officers’ identities are daily constructed and affirmed through their juxtaposition with inmates and the dominant gendered narratives. It also examines how stigma and preco
思考而得
发表于 2025-3-27 02:10:15
P. Notni,W. BronkallaArbeiten von Gale Miller (1992) und James Holstein (1992) (siehe auch Holstein/Miller 1993). Im Unterschied zu einer Vielzahl weiterer Ansätze im Forschungsbereich sozialer Probleme beschäftigen sie sich nicht mit gesellschaftlichen Definitionsprozessen, sondern mit „der Konstruktion konkreter Probl
悦耳
发表于 2025-3-27 06:05:47
P. C. van der Kruit,G. S. ShostakArbeiten von Gale Miller (1992) und James Holstein (1992) (siehe auch Holstein/Miller 1993). Im Unterschied zu einer Vielzahl weiterer Ansätze im Forschungsbereich sozialer Probleme beschäftigen sie sich nicht mit gesellschaftlichen Definitionsprozessen, sondern mit „der Konstruktion konkreter Probl
Debate
发表于 2025-3-27 11:20:41
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清澈
发表于 2025-3-27 17:15:11
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Fulsome
发表于 2025-3-27 18:53:36
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enterprise
发表于 2025-3-27 23:08:35
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不适
发表于 2025-3-28 02:07:07
HI Observations of the Irregular Galaxy IC 10De Vaucouleurs and Freeman (1972) have classified it as a Magellanic barred irregular. With a heliocentric radial velocity of -350 km/sec, its distance is uncertain, and various investigators have placed it as far away as 3, and as near as 1 Mpc (Bottinelli et al., 1972; Roberts, 1962). For the latt
搏斗
发表于 2025-3-28 08:04:31
The Distribution of Molecular Clouds in Spiral GalaxiesI is concentrated in the inner part of the Galaxy in a “ring” between 4–8 kpc and in the inner 1 kpc. Subsequent surveys (Gordon and Burton 1976, Cohen and Thaddeus 1977, Solomon .. {dy1979}) confirmed this picture with more extensive data. The molecular interstellar medium was shown to be dominated
Gossamer
发表于 2025-3-28 11:52:18
The CO Rotation Curve of the Milky Way : Accuracy and Implications= 18 kpc. Recently, Blitz and Fich (1983) have examined the uncertainties in the rotation curve at large R and have concluded that : 1) Of all the uncertainties, small changes in R. and θ. have the most serious effect on the rise at large R. However, unless ω. < 20 km s. kpc., a value smaller than t