scholarly journals SUTDIES ON SUB-FABRIC BURNS: THE RELATIONSHIP OF SURFACE APPEARANCE AND DEPTH OF DAMAGE A METHOD OF STUDY, PRELIMINARY RESULTS, AND OBSERVATIONS OF WOUND HEALING

1958 ◽  
Author(s):  
K. M. Berkley
Author(s):  
Jerry Gale

This brief report presents some preliminary results of part of a study currently being conducted (Gale, 1992, May). The study is a qualitative analysis of a couple's and therapist's perspective of meaningful moments in therapy using Interpersonal Process Recall (IPR) (Elliott, 1986). The methodology of this study involved the collaborators (aka: subjects) in a manner that was self-reflexive and recursive (see Steier, in press). The impact of the study was such that the research interviews themselves were reported to have greater therapeutic impact than the therapy. Following eight sessions of marital therapy, the couple reported that therapy was not helpful, and they were together only because of the children. Following the second IPR interview, which was post-therapy, the couple reported that the interview was very useful and therapeutic. This seemed to occur, in part, from three different factors. These factors include: the relationship of the couple to the researcher; the contextualization of the research talk; and clarifying procedures used by the interviewer.


1997 ◽  
Vol 170 ◽  
pp. 36-38
Author(s):  
Mark H. Heyer

FCRAO has initiated an imaging survey of CO J=1–0 emission from the outer Galaxy to better understand the physical properties of the molecular gas component of the interstellar medium and to determine the relationship of this component to spiral arm features. When completed in Spring 1996, the CO Survey will cover 103° < lII < 145°, −3° < bII < 5°, and −150 < VLSR < 50 km s–1 with angular sampling of 50″ and velocity resolution of 0.8 km s–1. During the first year of observations, we have focused upon two fields with longitude ranges of 103° < lII < 112° and 131° < lII < 139°. The first field corresponds to the Cepheus region while the second field contains the W3, W4, and W5 complex of HII regions. To date, 700,000 CO spectra have been collected. In this contribution, we present preliminary results from the first year of observations.


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