By Shapley H.
Read or Download [Article] Studies of Magnitudes in Star Clusters II. On the Sequence of Spectral Types in Stellar Evolution PDF
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Additional info for [Article] Studies of Magnitudes in Star Clusters II. On the Sequence of Spectral Types in Stellar Evolution
This binary pair corresponds to the oppositions between chora/Semiotic and Symbolic, and, by extension, between the pre-oedipal and oedipal phases. Because we inevitably inhabit Euclidean space, the customary common-sense space of everyday life, we have difficulty envisaging other spaces and the values that accompany them. This is, of course, the problem which underlies any attempt to represent that which precedes representation. As Kristeva does not tire of pointing out, the chora or Semiotic can only be known indirectly, by the manner in which they disturb or disrupt the Symbolic.
The terms with which she works are ambiguous. On the one hand, the model she constructs is a temporal one of early childhood development towards the acquisition of language and its concomitant logical processes. On the other hand, the countermodel she proposes, that of the “return of the repressed” Semiotic in the form of avant-garde artistic creation, is couched in spatial terms of eruption, effraction, displacement. In the ambiguous paradigms which underlie her dual model, what can be seen is the surging up of (deviant) space into (normative) temporality – an intrusion described in spatial terms.
In the course of our subsequent analyses, we will see that Kristeva gradually relinquishes this binary structure. One significant problem which Kristeva addresses is the peripherality of subversion: “By relegating the source of subversion to a site outside of culture itself, Kristeva appears to foreclose the possibility of subversion as an effective or realizable cultural practice. Pleasure beyond the paternal law can only be imagined together with its inevitable impossibility” (Butler 1990: 88).
[Article] Studies of Magnitudes in Star Clusters II. On the Sequence of Spectral Types in Stellar Evolution by Shapley H.