Liturgy and Ecumenism: What Next?

(Excerpt) This year, 1998, marks the twentieth anniversary of the Lutheran Book of Worship (LBW) that we celebrate together with the fiftieth anniversary of the Institute of Liturgical Studies here at Valparaiso University. My personal debt to the institute goes back to 1956 when I persuaded my internship supervisor to allow me to attend the institute in Michigan. That meeting introduced me to some of the giants of the previous generation-Arthur Carl Piepkorn, Berthold von Schenk, AR. Kretzmann and M. Alfred Bichsel-and gave me a vision of what worship among Lutherans might be. Then, following my return from doctoral studies at the University of Heidelberg, I was invited to present a paper at the 1961 institute. It was on the concept of anamnesis, prescient of this year\u27s eschatological theme. And now, after fifteen years as an ex-patriot, you have invited me back. I am grateful

Through My Eyes: The Effect on Family Life of Having Siblings with Autism Spectrum Disorder as Experienced by a Typically Developing Adolescent

As the prevalence of Autism Spectrum Disorder (ASD) continues to increase, research efforts have begun to focus on the effects a person with ASD has on family life. The dominant voice in the extant literature is that of parents and caregivers, but only a small body of research explores the experiences of siblings. Using a phenomenological approach, a qualitative study was conducted to understand how a typically developing (TD) adolescent experiences the effects of having siblings with ASD on family routines and activities. Findings indicate that the family’s performance context—including routines, relationships, and activities—acts as the mediator of the bidirectional relationship between the siblings with ASD’s person factors and the TD adolescent\u27s identity. These findings support the use of a family-centered approach in occupational therapy when working with individuals with ASD and tailoring interventions to support the needs of all

Through My Eyes: The Effect on Family Life of Having Siblings with Autism Spectrum Disorder as Experienced by a Typically Developing Adolescent

As the prevalence of Autism Spectrum Disorder (ASD) continues to increase, research efforts have begun to focus on the effects a person with ASD has on family life. The dominant voice in the extant literature is that of parents and caregivers, but only a small body of research explores the experiences of siblings. Using a phenomenological approach, a qualitative study was conducted to understand how a typically developing (TD) adolescent experiences the effects of having siblings with ASD on family routines and activities. Findings indicate that the family’s performance context—including routines, relationships, and activities—acts as the mediator of the bidirectional relationship between the siblings with ASD’s person factors and the TD adolescent\u27s identity. These findings support the use of a family-centered approach in occupational therapy when working with individuals with ASD and tailoring interventions to support the needs of all

Toward the Renewal of Christian Initiation in the Parish

(Excerpt) The brochure for this year\u27s Institute contained the arresting sentence: To discuss the question of Christian initiation is, finally, to inquire after the very nature of the church: the issue is of vast ecclesiological significance. The renewed and growing interest in Christian initiation is prompted by a new vision of the church

The relation between age at school entrance and achievement of pupils in five New Hampshire towns in grades one through six

Thesis (Ed.M.)--Boston Universit

Molecular gas and stars in the translucent cloud MBM 18 (LDN 1569)

Seven of ten candidate H-alpha emission-line stars found in an objective grism survey of a 1 square degree region in MBM 18, were observed spectroscopically. Four of these have weak H-alpha emission, and 6 out of 7 have spectral types M1-M4V. One star is of type F7-G1V, and has H-alpha in absorption. The spectra of three of the M-stars may show an absorption line of LiI, although none of these is an unambiguous detection. For the six M-stars a good fit is obtained with pre-main-sequence isochrones indicating ages between 7.5 and 15Myr. The molecular cloud mass, derived from the integrated 12CO(1-0) emission, is 160Mo (for a distance of 120pc), much smaller than the virial mass (10^3Mo), and the cloud is not gravitationally bound. Nor are the individual clumps we identified through a clump-finding routine. Considering the relative weakness or absence of the H-alpha emission, the absence of other emission lines, and the lack of clear LiI absorption, the targets are not T Tauri stars. With ages between 7.5 and 15Myr they are old enough to explain the lack of lithium in their spectra. Based on the derived distances (60-250pc), some of the stars may lie inside the molecular cloud (120-150pc). From the fact that the cloud as a whole, as well as the individual clumps, are not gravitationally bound, in combination with the ages of the stars we conclude that it is not likely that (these) stars were formed in MBM 18.Comment: Accepted for publication in Astronomy & Astrophysics (20 pages