VI. Regrouping Social Identities

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/66578/2/10.1177_0959353599009003009.pd

Resisting Gendered Smoking Pressures: Critical Consciousness as a Correlate of Women's Smoking Status

Gender is one of the social structures, along with social class and ethnicity, that shapes women's smoking behaviors. We examined how different responses to gender pressures (internalization and resistance) relate to smoking. We analyzed data from a national random digit dial survey of 945 women and found that never smokers scored high on resistance to gender pressure (indicated by high scores on feminist consciousness) and on education and Body Mass Index; current smokers had the reverse pattern. Ex-smokers scored high on one measure of resistance (advertising skepticism) and on two measures of internalization (embodied femininity and weight concern); they were also likely to have high household income and to be European American. Results are discussed in terms of their implications for smoking cessation programs and antismoking campaigns.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/45642/1/11199_2005_Article_5684.pd

Mapping Distances Across the Perseus Molecular Cloud Using CO Observations, Stellar Photometry, and Gaia DR2 Parallax Measurements

We present a new technique to determine distances to major star-forming regions across the Perseus Molecular Cloud, using a combination of stellar photometry, astrometric data, and $\rm ^{12} CO$ spectral-line maps. Incorporating the Gaia DR2 parallax measurements when available, we start by inferring the distance and reddening to stars from their Pan-STARRS1 and 2MASS photometry, based on a technique presented in Green et al. 2014; Green et al. 2015 and implemented in their 3D "Bayestar" dust map of three-quarters of the sky. We then refine the Green et al. technique by using the velocity slices of a CO spectral cube as dust templates and modeling the cumulative distribution of dust along the line of sight towards these stars as a linear combination of the emission in the slices. Using a nested sampling algorithm, we fit these per-star distance-reddening measurements to find the distances to the CO velocity slices towards each star-forming region. This results in distance estimates explicitly tied to the velocity structure of the molecular gas. We determine distances to the B5, IC348, B1, NGC1333, L1448, and L1451 star-forming regions and find that individual clouds are located between $\approx 275-300$ pc, with typical combined uncertainties of $\approx 5\%$. We find that the velocity gradient across Perseus corresponds to a distance gradient of about 25 pc, with the eastern portion of the cloud farther away than the western portion. We determine an average distance to the complex of $294\pm 17$ pc, about 60 pc higher than the distance derived to the western portion of the cloud using parallax measurements of water masers associated with young stellar objects. The method we present is not limited to the Perseus Complex, but may be applied anywhere on the sky with adequate CO data in the pursuit of more accurate 3D maps of molecular clouds in the solar neighborhood and beyond.Comment: Accepted for publication in The Astrophysical Journa

Relative Alignment between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud Using Low- and High-density Tracers

We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500 μm polarization maps made with the BLASTPol balloon-borne polarimeter to the orientation of structures in the integrated line emission maps from Mopra observations. Averaging over the entire cloud we find that elongated structures in integrated line-intensity or zeroth-moment maps, for low-density tracers such as 12CO and 13CO J → 1 – 0, are statistically more likely to align parallel to the magnetic field, while intermediate- or high-density tracers show (on average) a tendency for alignment perpendicular to the magnetic field. This observation agrees with previous studies of the change in relative orientation with column density in Vela C, and supports a model where the magnetic field is strong enough to have influenced the formation of dense gas structures within Vela C. The transition from parallel to no preferred/perpendicular orientation appears to occur between the densities traced by 13CO and by C18O J → 1 – 0. Using RADEX radiative transfer models to estimate the characteristic number density traced by each molecular line, we find that the transition occurs at a molecular hydrogen number density of approximately 103 cm−3. We also see that the Centre Ridge (the highest column density and most active star-forming region within Vela C) appears to have a transition at a lower number density, suggesting that this may depend on the evolutionary state of the cloud

College-educated women's personality development in adulthood: Perceptions and age differences.

Adulthood encompasses a large time span and includes a series of psychosocial challenges (E. H. Erikson, 1950). Five aspects of personality (identity certainty, confident power, concern with aging, generativity, and personal distress) were assessed in a cross-sectional study of college-educated women who at the time of data collection were young adults (age: M 26 years), middle-aged adults (age: M 46 years), or older adults (age: M 66 years). Respondents rated each personality domain for how true it was of them at the time, and they then rated the other 2 ages either retrospectively or prospectively. Results are discussed with attention to the ways in which women’s adult development may have been shaped by experiences particular to both gender and birth cohort, and to how these women fit with E. H. Erikson’s theory of adult development. The developmental period of adulthood covers a large time span, from age 18 or 21 to death. A variety of strategies for dividing this long period into shorter age-based periods have been recommended. For example, Erikson’s (1950) theory of psycho-social development includes distinctive stages defined by person-ality developmental tasks; for example, young adulthood (the 20s) is characterized as a time of concern with identity and intimacy issues, whereas middle age (the 40s) is characterized as a time of concern with generativity. Other theorists (e.g., Neugarten, 1968) have emphasized the notion of “executive personality ” in middle age, or a confident sense of command. Older adulthood in Erik-son’s theory is characterized as a time of personality integration in which the key accomplishment is a sense of integrity. Recent theorists have noted that these issues (identity, intimacy, genera-tivity, and integrity) preoccupy adults to varying degrees at all ages, although they may be particularly intense during specific periods and may take different forms at different adult ages (e.g.

Tracking Homo Oeconomicus: Development of the Neoliberal Beliefs Inventory

Researchers across the social sciences are beginning to note that neoliberalism’s influence is no longer restricted to macroeconomic and social policies, but can now be detected in individuals’ behaviors, relationships, perceptions, and self-concept. However, psychologists lack a means of assessing neoliberal beliefs directly. We collected data from three samples of U.S. undergraduates to develop and test a measure of neoliberal ideology, the Neoliberal Beliefs Inventory (NBI). Using first exploratory and then confirmatory factor analysis, we devised a 25-item measure that is both reliable and valid, at least within a particular demographic (i.e., U.S. traditionally-aged undergraduates). The NBI may help psychologists specify and analyze the role of neoliberal ideology in shaping human behavior and functioning