242 research outputs found
Observations of the 6 Centimeter Lines of OH in Evolved (OH/IR) Stars
Recent observational and theoretical advances have called into question
traditional OH maser pumping models in evolved (OH/IR) stars. The detection of
excited-state OH lines would provide additional constraints to discriminate
amongst these theoretical models. In this Letter, we report on VLA observations
of the 4750 MHz and 4765 MHz lines of OH toward 45 sources, mostly evolved
stars. We detect 4765 MHz emission in the star forming regions Mon R2 and LDN
1084, but we do not detect excited-state emission in any evolved stars. The
flux density and velocity of the 4765 MHz detection in Mon R2 suggests that a
new flaring event has begun.Comment: 4 pages, to appear in ApJ
The Nature of Composite LINER/HII Galaxies, As Revealed from High-Resolution VLA Observations
A sample of 37 nearby galaxies displaying composite LINER/HII and pure HII
spectra was observed with the VLA in an investigation of the nature of their
weak radio emission. The resulting radio contour maps overlaid on optical
galaxy images are presented here, together with an extensive literature list
and discussion of the individual galaxies. Radio morphological data permit
assessment of the ``classical AGN'' contribution to the global activity
observed in these ``transition'' LINER galaxies. One in five of the latter
objects display clear AGN characteristics: these occur exclusively in
bulge-dominated hosts.Comment: 31 pages, 27 figures, accepted by ApJ
IL-12p35 induces expansion of IL-10 and IL-35-expressing regulatory B cells and ameliorates autoimmune disease
We thank Dr. Haohua Qian and Yichao Li (Visual function core, NEI, NIH) for technical assistance with OCT; Phyllis Silver (NEI, NIH) for EAU scoring of the eyes; Rashid Mahdi. M.J.M. for technical assistance with western blot analyses and Rafael Villasmil (NEI FLOW Cytometry Core facility) for assistance with FACS analysis.Peer reviewedPublisher PD
IL-35 Is a Novel Responsive Anti-inflammatory Cytokine — A New System of Categorizing Anti-inflammatory Cytokines
It remains unknown whether newly identified anti-inflammatory/immunosuppressive cytokine interleukin-35 (IL-35) is different from other anti-inflammatory cytokines such as IL-10 and transforming growth factor (TGF)-β in terms of inhibition of inflammation initiation and suppression of full-blown inflammation. Using experimental database mining and statistical analysis methods we developed, we examined the tissue expression profiles and regulatory mechanisms of IL-35 in comparison to other anti-inflammatory cytokines. Our results suggest that in contrast to TGF-β, IL-35 is not constitutively expressed in human tissues but it is inducible in response to inflammatory stimuli. We also provide structural evidence that AU-rich element (ARE) binding proteins and microRNAs target IL-35 subunit transcripts, by which IL-35 may achieve non-constitutive expression status. Furthermore, we propose a new system to categorize anti-inflammatory cytokines into two groups: (1) the house-keeping cytokines, such as TGF-β, inhibit the initiation of inflammation whereas (2) the responsive cytokines including IL-35 suppress inflammation in full-blown stage. Our in-depth analyses of molecular events that regulate the production of IL-35 as well as the new categorization system of anti-inflammatory cytokines are important for the design of new strategies of immune therapies
ISOCAM view of the starburst galaxies M82, NGC253, and NGC1808
We present results of mid-infrared 5.0-16.5 micron spectrophotometric imaging
of the starburst galaxies M82, NGC253, and NGC1808 from the ISOCAM instrument
on board the Infrared Space Observatory. The mid-infrared spectra of the three
galaxies are very similar in terms of features present. The > 11 micron
continuum attributed to very small dust grains (VSGs) exhibits a large spread
in intensity relative to the short-wavelength emission. We find that the 15
micron dust continuum flux density correlates well with the fine-structure
[ArII] 6.99 micron line flux and thus provides a good quantitative indicator of
the level of star formation activity. By contrast, the 5-11 micron region
dominated by emission from polycyclic aromatic hydrocarbons (PAHs) has a nearly
invariant shape. Variations in the relative intensities of the PAH features are
nevertheless observed, at the 20%-100% level. We illustrate extinction effects
on the shape of the mid-infrared spectrum of obscured starbursts, emphasizing
the differences depending on the applicable extinction law and the consequences
for the interpretation of PAH ratios and extinction estimates. The relative
spatial distributions of the PAH, VSG, and [ArII] 6.99 micron emission between
the three galaxies exhibit remarkable differences. The < 1 kpc size of the
mid-infrared source is much smaller than the optical extent of our sample
galaxies and 70%-100% of the IRAS 12 micron flux is recovered within the ISOCAM
< 1.5 arcmin squared field of view, indicating that the nuclear starburst
dominates the total mid-infrared emission while diffuse light from quiescent
disk star formation contributes little.Comment: 25 pages, 12 figures, accepted for publication in Astronomy and
Astrophysics; Figs. 3, 4, 5, 6, 7, 9, 10, 12 appear after Sect.
The Rachel Carson Letters and the Making of Silent Spring
Environment, conservation, green, and kindred movements look back to Rachel Carson’s 1962 book Silent Spring as a milestone. The impact of the book, including on government, industry, and civil society, was immediate and substantial, and has been extensively described; however, the provenance of the book has been less thoroughly examined. Using Carson’s personal correspondence, this paper reveals that the primary source for Carson’s book was the extensive evidence and contacts compiled by two biodynamic farmers, Marjorie Spock and Mary T. Richards, of Long Island, New York. Their evidence was compiled for a suite of legal actions (1957-1960) against the U.S. Government and that contested the aerial spraying of dichlorodiphenyltrichloroethane (DDT). During Rudolf Steiner’s lifetime, Spock and Richards both studied at Steiner’s Goetheanum, the headquarters of Anthroposophy, located in Dornach, Switzerland. Spock and Richards were prominent U.S. anthroposophists, and established a biodynamic farm under the tutelage of the leading biodynamics exponent of the time, Dr. Ehrenfried Pfeiffer. When their property was under threat from a government program of DDT spraying, they brought their case, eventually lost it, in the process spent US$100,000, and compiled the evidence that they then shared with Carson, who used it, and their extensive contacts and the trial transcripts, as the primary input for Silent Spring. Carson attributed to Spock, Richards, and Pfeiffer, no credit whatsoever in her book. As a consequence, the organics movement has not received the recognition, that is its due, as the primary impulse for Silent Spring, and it is, itself, unaware of this provenance
Mid-Infrared Imaging of Active Galaxies: Active Nuclei and Embedded Star Clusters
High resolution, mid-infrared (MIR) images of a set of nine nearby active
galaxies are presented. The data were obtained with the TIMMI2 instrument
mounted at the ESO 3.6m telescope using a set of N-band narrow filters. The
resulting images have an angular resolution of 0.6"-1". The MIR emission has
been resolved in four galaxies: NGC253, NGC1365, NGC1808 and NGC7469. The
images unveil a circumnuclear population of unknown MIR sources in NGC1365 and
NGC1808, coincident with radio sources. These MIR/radio sources are interpreted
in terms of embedded young star clusters. A high-resolution MIR map of NGC253
is also presented, and enables the identification of a previously unknown MIR
counterpart to the radio nucleus. Extended MIR emission is detected in NGC7469,
and concurs with previous observations in the NIR and radio. For this source,
an interesting morphological difference between the 10.4mic and the 11.9mic
emission is observed, suggesting the presence of a dust-rich micro-bar. Our MIR
images of Circinus do not show resolved emission from the nucleus down to an
angular scale of 0.5". In the case of NGC2992, an upper limit to the extended
MIR emission can be set. Finally, we provide new MIR flux measurements for the
unresolved AGN in NGC5995, IZw1 and IIZw136.Comment: 19 pages, 11 figures, accepted for publication in A&
Nothing New in the (North) East? Interpreting the Rhetoric and Reality of Japanese Corporate Governance
Japan finally seems to be pulling itself out of its lost decade (and a half) of economic stagnation. Some grudgingly or triumphantly attribute this to micro-economic reforms, freeing up arthritic markets, although there is also evidence that macro-economic policy failures have been a major cause of poor performance since the 1990s. Many point to overlapping transformations in corporate governance, broadly defined to cover relationships among managers and employees as well as between firms and outside shareholders, creditors, and other stakeholders. These relationships are in flux, with moves arguably favouring shareholders and more market-driven control mechanisms. It has certainly been a found decade for law reform in Japan, particularly in corporate law, with a plethora of legislative amendments commencing around 1993 and culminating in the enactment of a consolidated Company Law in 2005. This modernisation project, particularly since 2001, is reportedly aimed at (i) securing better corporate governance, (ii) bringing the law into line with a highly-developed information society, (iii) liberalising fundraising measures, (iv) bringing corporate law into line with the internationalization of corporate activity, and (v) modernizing terms and consolidating corporate law. Because the suite of revisions has moved away from strict mandatory rules set out originally in Japan\u27s Commercial Code of 1899, modeled primarily on German law, another growing perception is that Japanese corporate law and practice is or will soon be converging significantly on US models. However, assessments remain divided as to whether these moves in corporate governance and capitalism more generally in Japan amount to a new paradigm or regime shift . Focusing primarily on quite influential commentary in English, Part I of this paper outlines two pairs of views. It concludes that the most plausible assessment is of significant but gradual transformation towards a more market-driven approach, evident also in other advanced political economies. Drawing more generally from these often virulently divided views, Part II sets out five ways forward through the proliferating literature and source material on corporate governance in Japan. Particular care must be taken in: (i) selecting the temporal timeframe, (ii) selecting countries to compare, (iii) balancing black-letter law and broader socio-economic context, (iv) reflecting on and disclosing normative preferences, and (v) giving weight to processes as well as outcomes, when assessing change in Japan - and any other country\u27s governance system. Part III ends with a call for further research particularly on law- and policy-producing processes, rather than mainly outcomes. It also outlines the usefulness of this analytical framework for analysing the broader field of Corporate Social Responsibility, now emerging as the next major area of debate and transformation in Japan - as elsewhere
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