The 1980s—Best Friends Again. One Is Shooting, the Other Is Collapsing.

Forty-eight introductory psychology students (28 females, 20 males) and their same-sex best friends participated in this study. Based upon a question from the Adult Attachment Interview (George, Kaplan, & Main, 1996), participants wrote five adjectives that described their childhood relationships with each parent. For the four most descriptive adjectives (two for mothers and two for fathers), they wrote about childhood incidents that illustrated those adjectives. Adjectives were evaluated for how positively participants described their relationships with mothers and with fathers; incidents were evaluated for how loving, rejecting, and neglectful mothers and fathers appeared to have been during childhood. Next, best friend pairs participated in a series of videotaped conversation tasks where they discussed unresolved problems. Those who recalled more loving mothers were better able to disclose intimate personal information to their friends and to clearly express their feelings about their problems.Those who recalled more neglectful mothers, on the other hand, were more likely to exhibit heightened emotionality when discussing their problems. Implications for future research are discussed.

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Finding Fran

American Journal of Islam and Society ◽

10.35632/ajis.v18i4.1986 ◽

2001 ◽

Vol 18 (4) ◽

pp. 140-143

Author(s):

Gretchen Iman Meyer-Hoffman

Keyword(s):

High School ◽

New Mexico ◽

The Other ◽

College Life ◽

Feminist History ◽

Best Friends ◽

The Third ◽

Personal Nature ◽

Artistically Talented ◽

Sufi Order

Finding Fran is a memoir of two women, once best friends, who take verydifferent paths. The author is now a feminist history professor and her highschool friend, Fran, is Noura-a Muslim living in Egypt Banner looksback on their lives to find out what led one to feminism and the other toIslam. Unfortunately, while Banner offers many interesting insights into thelives of both women, she never fully answers this fundamental question.The book is divided into four parts. Part I, "My Story (1944-1952),"explores Banner's family history as well as her life up Wltil high school. Shetraces the lives of various family members in order to discover how theyaffected her childhood and her outlook on life. In the second part, "Fran &Me (1952-1956)," Banner tells the story of their high school friendship.It is a friendship of two smart and artistically talented girls, who are oftenbold and passionate in a time and place that glorified passive, femininewomen. Together they navigate the seemingly esoteric system of footballplayers and prom queens without ever really belonging to that system.In college they separate, Banner to UCLA and Fran to Stanford. This isthe beginning of their two different paths. Banner takes to academia andfeminism, while Fran is drawn to the various spiritual movements of the1960s. These years are covered in the third section, "Passages (1956-1982)." Banner includes chapters on their college life and the yearsimmediately following, and then delves into her life as an academic and afeminist.The last section covers Fran/Noura's life between 1967 and 1990. Shestudies Zen and other spiritual movements, such as the Gurdjieff system. Inlate 1960s, she moves to a commune in New Mexico. There she discoverswesternized Sufi practices that have been cut from their Islamic base. Hercontinuing quest leads her to study Islam. She eventually becomes aMuslim and a member of a traditional Sufi order. Later, she studies in SaudiArabia, and currently, she residues in Egypt.In keeping with the personal nature of the book, Banner includes acollection of photographs ranging from old family snapshots to the twowomen together in high school in 1956 and again in Egypt in 1992. Muchof Banner's analysis comes in the prologue and the epilogue. She alsoincludes detailed notes for each chapter ...

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Stromatoporoids from the Famennian (Devonian) Wabamun Formation, Normandville oilfield, north–central Alberta, Canada

Journal of Paleontology ◽

10.1017/s0022336000018321 ◽

1988 ◽

Vol 62 (03) ◽

pp. 411-419 ◽

Cited By ~ 5

Author(s):

Colin W. Stearn

Keyword(s):

Patch Reef ◽

Abundant Species ◽

The Other ◽

North Central ◽

Biotic Crisis

Stromatoporoids are the principal framebuilding organisms in the patch reef that is part of the reservoir of the Normandville field. The reef is 10 m thick and 1.5 km2in area and demonstrates that stromatoporoids retained their ability to build reefal edifices into Famennian time despite the biotic crisis at the close of Frasnian time. The fauna is dominated by labechiids but includes three non-labechiid species. The most abundant species isStylostroma sinense(Dong) butLabechia palliseriStearn is also common. Both these species are highly variable and are described in terms of multiple phases that occur in a single skeleton. The other species described areClathrostromacf.C. jukkenseYavorsky,Gerronostromasp. (a columnar species), andStromatoporasp. The fauna belongs in Famennian/Strunian assemblage 2 as defined by Stearn et al. (1988).

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D. The Line Spectrum of Pulsating Variable Stars

Symposium - International Astronomical Union ◽

10.1017/s0074180900019021 ◽

1967 ◽

Vol 28 ◽

pp. 207-244

Author(s):

R. P. Kraft

Keyword(s):

Variable Stars ◽

The Other ◽

Line Spectrum ◽

Afternoon Session ◽

Empirical Information ◽

Pulsating Variable Stars ◽

Almost Continuous ◽

Informal Approach

(Ed. note:Encouraged by the success of the more informal approach in Christy's presentation, we tried an even more extreme experiment in this session, I-D. In essence, Kraft held the floor continuously all morning, and for the hour and a half afternoon session, serving as a combined Summary-Introductory speaker and a marathon-moderator of a running discussion on the line spectrum of cepheids. There was almost continuous interruption of his presentation; and most points raised from the floor were followed through in detail, no matter how digressive to the main presentation. This approach turned out to be much too extreme. It is wearing on the speaker, and the other members of the symposium feel more like an audience and less like participants in a dissective discussion. Because Kraft presented a compendious collection of empirical information, and, based on it, an exceedingly novel series of suggestions on the cepheid problem, these defects were probably aggravated by the first and alleviated by the second. I am much indebted to Kraft for working with me on a preliminary editing, to try to delete the side-excursions and to retain coherence about the main points. As usual, however, all responsibility for defects in final editing is wholly my own.)

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C. The Continuous Spectrum of Pulsating Variable Stars

Symposium - International Astronomical Union ◽

10.1017/s007418090001901x ◽

1967 ◽

Vol 28 ◽

pp. 177-206

Author(s):

J. B. Oke ◽

C. A. Whitney

Keyword(s):

Continuous Spectrum ◽

Variable Stars ◽

Velocity Fields ◽

The Other ◽

Line Spectrum ◽

Direct Information ◽

Thermodynamic Structure ◽

Diagnostic Interpretation ◽

Pulsating Variable Stars ◽

The Continuum

Pecker:The topic to be considered today is the continuous spectrum of certain stars, whose variability we attribute to a pulsation of some part of their structure. Obviously, this continuous spectrum provides a test of the pulsation theory to the extent that the continuum is completely and accurately observed and that we can analyse it to infer the structure of the star producing it. The continuum is one of the two possible spectral observations; the other is the line spectrum. It is obvious that from studies of the continuum alone, we obtain no direct information on the velocity fields in the star. We obtain information only on the thermodynamic structure of the photospheric layers of these stars–the photospheric layers being defined as those from which the observed continuum directly arises. So the problems arising in a study of the continuum are of two general kinds: completeness of observation, and adequacy of diagnostic interpretation. I will make a few comments on these, then turn the meeting over to Oke and Whitney.

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Observing programme for the 24-inch/36-inch Schmidt telescope

Symposium - International Astronomical Union ◽

10.1017/s007418090005364x ◽

1966 ◽

Vol 24 ◽

pp. 337

Author(s):

W. Iwanowska

Keyword(s):

The Other ◽

Schmidt Telescope ◽

Flint Glass

A new 24-inch/36-inch//3 Schmidt telescope, made by C. Zeiss, Jena, has been installed since 30 August 1962, at the N. Copernicus University Observatory in Toruń. It is equipped with two objective prisms, used separately, one of crown the other of flint glass, each of 5° refracting angle, giving dispersions of 560Å/mm and 250Å/ mm respectively.

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A hard choice for Tomasello

Behavioral and Brain Sciences ◽

10.1017/s0140525x19002346 ◽

2020 ◽

Vol 43 ◽

Author(s):

Philip Pettit

Keyword(s):

Joint Action ◽

The Other ◽

Hard Choice ◽

Margaret Gilbert ◽

Michael Bratman ◽

Human Sense ◽

Sense Of Obligation

Abstract Michael Tomasello explains the human sense of obligation by the role it plays in negotiating practices of acting jointly and the commitments they underwrite. He draws in his work on two models of joint action, one from Michael Bratman, the other from Margaret Gilbert. But Bratman's makes the explanation too difficult to succeed, and Gilbert's makes it too easy.

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A study of cometary eruptions through OH radio-lines

International Astronomical Union Colloquium ◽

10.1017/s025292110003150x ◽

1999 ◽

Vol 173 ◽

pp. 249-254

Author(s):

A.M. Silva ◽

R.D. Miró

Keyword(s):

Short Duration ◽

Growth Curves ◽

The Other ◽

Initial Mass ◽

Radio Lines ◽

Other Hand ◽

Sudden Rise

AbstractWe have developed a model for theH2OandOHevolution in a comet outburst, assuming that together with the gas, a distribution of icy grains is ejected. With an initial mass of icy grains of 108kg released, theH2OandOHproductions are increased up to a factor two, and the growth curves change drastically in the first two days. The model is applied to eruptions detected in theOHradio monitorings and fits well with the slow variations in the flux. On the other hand, several events of short duration appear, consisting of a sudden rise ofOHflux, followed by a sudden decay on the second day. These apparent short bursts are frequently found as precursors of a more durable eruption. We suggest that both of them are part of a unique eruption, and that the sudden decay is due to collisions that de-excite theOHmaser, when it reaches the Cometopause region located at 1.35 × 105kmfrom the nucleus.

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Note on Selection of Coordinate Systems for Geodynamics

International Astronomical Union Colloquium ◽

10.1017/s0252921100051174 ◽

1975 ◽

Vol 26 ◽

pp. 395-407

Author(s):

S. Henriksen

Keyword(s):

Sea Level ◽

The Other ◽

Coordinate Systems ◽

Mean Sea Level ◽

The Earth ◽

The One ◽

Static Systems ◽

Selection Of

The first question to be answered, in seeking coordinate systems for geodynamics, is: what is geodynamics? The answer is, of course, that geodynamics is that part of geophysics which is concerned with movements of the Earth, as opposed to geostatics which is the physics of the stationary Earth. But as far as we know, there is no stationary Earth – epur sic monere. So geodynamics is actually coextensive with geophysics, and coordinate systems suitable for the one should be suitable for the other. At the present time, there are not many coordinate systems, if any, that can be identified with a static Earth. Certainly the only coordinate of aeronomic (atmospheric) interest is the height, and this is usually either as geodynamic height or as pressure. In oceanology, the most important coordinate is depth, and this, like heights in the atmosphere, is expressed as metric depth from mean sea level, as geodynamic depth, or as pressure. Only for the earth do we find “static” systems in use, ana even here there is real question as to whether the systems are dynamic or static. So it would seem that our answer to the question, of what kind, of coordinate systems are we seeking, must be that we are looking for the same systems as are used in geophysics, and these systems are dynamic in nature already – that is, their definition involvestime.

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Discussion of the Oblique Rotator Model Cases Of 108 Aqr and x Serp.

International Astronomical Union Colloquium ◽

10.1017/s0252921100080891 ◽

1976 ◽

Vol 32 ◽

pp. 577-588

Author(s):

C. Mégessier ◽

V. Khokhlova ◽

T. Ryabchikova

Keyword(s):

Mathematical Formulation ◽

The Other ◽

Rotator Model ◽

Oblique Rotator ◽

First Results

My talk will be on the oblique rotator model which was first proposed by Stibbs (1950), and since received success and further developments. I shall present two different attempts at describing a star according to this model and the first results obtained in the framework of a Russian-French collaboration in order to test the precision of the two methods. The aim is to give the best possible representation of the element distributions on the Ap stellar surfaces. The first method is the mathematical formulation proposed by Deutsch (1958-1970) and applied by Deutsch (1958) to HD 125248, by Pyper (1969) to α2CVn and by Mégessier (1975) to 108 Aqr. The other one was proposed by Khokhlova (1974) and used by her group.

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