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The Roles of Interference and Inference In The Retrieval Of Autobiographical Memories
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The Evolution of Knowledge Representations with Increasing Expertise in Using Systems
Note and Comment
Waiver of the Statutory Protection to the confidential Relation of Physician and Patient; Inter-State Rendition; When a Public Officer Misappropriating Public Funds is Not an Embezzler; When a Discharged Teacher May Resort to the Courts
Bostonia. Volume 12
Founded in 1900, Bostonia magazine is Boston University's main alumni publication, which covers alumni and student life, as well as university activities, events, and programs
P Cygni Profiles of Molecular Lines Toward Arp 220 Nuclei
We report ~100 pc (0farcs3) resolution observations of (sub)millimeter HCO+ and CO lines in the ultraluminous infrared galaxy Arp 220. The lines peak at two merger nuclei, with HCO+ being more spatially concentrated than CO. Asymmetric line profiles with blueshifted absorption and redshifted emission are discovered in HCO+(3-2) and (4-3) toward the two nuclei and in CO(3-2) toward one nucleus. We suggest that these P Cygni profiles are due to ~100 km s–1 outward motion of molecular gas from the nuclei. This gas is most likely outflowing from the inner regions of the two nuclear disks rotating around individual nuclei, clearing the shroud around the luminosity sources there
Primordial Star Formation under Far-ultraviolet radiation
Thermal and chemical evolution of primordial gas clouds irradiated with
far-ultraviolet (FUV; < 13.6 eV) radiation is investigated. In clouds
irradiated by intense FUV radiation, sufficient hydrogen molecules to be
important for cooling are never formed. However, even without molecular
hydrogen, if the clouds are massive enough, they start collapsing via atomic
hydrogen line cooling. Such clouds continue to collapse almost isothermally
owing to successive cooling by H^{-} free-bound emission up to the number
density of 10^{16} cm^{-3}. Inside the clouds, the Jeans mass eventually falls
well below a solar mass. This indicates that hydrogen molecules are dispensable
for low-mass primordial star formation, provided fragmentation of the clouds
occurs at sufficiently high density.Comment: 32 pages and 9 figures. ApJ, in pres
Brief of Corporate Law Professors as Amici Curie in Support of Respondents
The Supreme Court has looked to the rights of corporate shareholders in determining the rights of union members and non-members to control political spending, and vice versa. The Court sometimes assumes that if shareholders disapprove of corporate political expression, they can easily sell their shares or exercise control over corporate spending. This assumption is mistaken. Because of how capital is saved and invested, most individual shareholders cannot obtain full information about corporate political activities, even after the fact, nor can they prevent their savings from being used to speak in ways with which they disagree. Individual shareholders have no “opt out” rights or practical ability to avoid subsidizing corporate political expression with which they disagree. Nor do individuals have the practical option to refrain from putting their savings into equity investments, as doing so would impose damaging economic penalties and ignore conventional financial guidance for individual investors
Repeat coronary angioplasty: Correlates of a second restenosis
AbstractTo identify the correlates of a second restenosis after repeat percutaneous coronary angioplasty, the records of 384 patients with single vessel disease who underwent repeat angioplasty for restenosis complicating a first elective angioplasty were examined. A second restenosis occurred in 47 (31%) of 151 patients having angiographic follow-up. Univariate correlates of a second restenosis were an interval between the first and the second angioplasty <5 months (41 versus 20% of patients had restenosis, p < 0.01), male gender (35 versus 12%, p < 0.05), lesion length ≥15 mm before the second angioplasty (62 versus 28%, p < 0.05), diameter stenosis >90% before the second angioplasty (67 versus 29%, p < 0.05), final gradient >20 mm Hg after the second angioplasty (52 versus 28%, p < 0.05) and an additional site requiring dilation at the time of the second angioplasty (50 versus 29%, p = 0.10).Multivarlate predictors of a second restenosis were an interval of <5 months between the first and the second angioplasty (p = 0.001), male gender (p = 0.001), lesion length ≥15 mm before the second angioplasty (p = 0.001) and the need to have an additional site dilated at the time of the second angioplasty (p = 0.002). Patients at increased risk of restenosis after the second angioplasty can be identified and may serve as a useful population for intervention studies
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