Very cold and massive cores near ISOSS J18364-0221: Implications for the initial conditions of high-mass star-formation

We report the discovery of two very cold and massive molecular cloud cores in the region ISOSS J18364-0221. The object has been identified by a systematic search for very early evolutionary stages of high-mass stars using the 170 micron ISOPHOT Serendipity Survey (ISOSS). Submm continuum and molecular line measurements reveal two compact cores within this region. The first core has a temperature of 16.5 K, shows signs of ongoing infall and outflows, has no NIR or MIR counterpart and is massive enough (M ~ 75 M_sun) to form at least one O star with an associated cluster. It is therefore considered a candidate for a genuine high-mass protostar and a high-mass analog to the Class 0 objects. The second core has an average gas and dust temperature of only ~ 12 K and a mass of M ~ 280 M_sun. Its temperature and level of turbulence are below the values found for massive cores so far and are suggested to represent the initial conditions from which high-mass star formation occurs.Comment: 9 pages, 6 figures, accepted for publication in the Astrophysical Journa

Dust Temperatures in the Infrared Space Observatory Atlas of Bright Spiral Galaxies

We examine far-infrared and submillimeter spectral energy distributions for galaxies in the Infrared Space Observatory Atlas of Bright Spiral Galaxies. For the 71 galaxies where we had complete 60-180 micron data, we fit blackbodies with lambda^-1 emissivities and average temperatures of 31 K or lambda^-2 emissivities and average temperatures of 22 K. Except for high temperatures determined in some early-type galaxies, the temperatures show no dependence on any galaxy characteristic. For the 60-850 micron range in eight galaxies, we fit blackbodies with lambda^-1, lambda-2, and lambda^-beta (with beta variable) emissivities to the data. The best results were with the lambda^-beta emissivities, where the temperatures were ~30 K and the emissivity coefficient beta ranged from 0.9 to 1.9. These results produced gas to dust ratios that ranged from 150 to 580, which were consistent with the ratio for the Milky Way and which exhibited relatively little dispersion compared to fits with fixed emissivities.Comment: AJ, 2003, in pres

First Measurement of the Atomic Electric Dipole Moment of \u3csup\u3e225\u3c/sup\u3eRa

The radioactive radium-225 (225Ra) atom is a favorable case to search for a permanent electric dipole moment. Because of its strong nuclear octupole deformation and large atomic mass, 225Ra is particularly sensitive to interactions in the nuclear medium that violate both time-reversal symmetry and parity. We have developed a cold-atom technique to study the spin precession of 225Ra atoms held in an optical dipole trap, and demonstrated the principle of this method by completing the first measurement of its atomic electric dipole moment, reaching an upper limit of |d(225Ra)|\u3c5.0×10−22  e cm (95% confidence)

Star-forming cores embedded in a massive cold clump: Fragmentation, collapse and energetic outflows

The fate of massive cold clumps, their internal structure and collapse need to be characterised to understand the initial conditions for the formation of high-mass stars, stellar systems, and the origin of associations and clusters. We explore the onset of star formation in the 75 M_sun SMM1 clump in the region ISOSS J18364-0221 using infrared and (sub-)millimetre observations including interferometry. This contracting clump has fragmented into two compact cores SMM1 North and South of 0.05 pc radius, having masses of 15 and 10 M_sun, and luminosities of 20 and 180 L_sun. SMM1 South harbours a source traced at 24 and 70um, drives an energetic molecular outflow, and appears supersonically turbulent at the core centre. SMM1 North has no infrared counterparts and shows lower levels of turbulence, but also drives an outflow. Both outflows appear collimated and parsec-scale near-infrared features probably trace the outflow-powering jets. We derived mass outflow rates of at least 4E-5 M_sun/yr and outflow timescales of less than 1E4 yr. Our HCN(1-0) modelling for SMM1 South yielded an infall velocity of 0.14 km/s and an estimated mass infall rate of 3E-5 M_sun/yr. Both cores may harbour seeds of intermediate- or high-mass stars. We compare the derived core properties with recent simulations of massive core collapse. They are consistent with the very early stages dominated by accretion luminosity.Comment: Accepted for publication in ApJ, 14 pages, 7 figure

No cold dust within the supernova remnant Cassiopeia A

A large amount (about three solar masses) of cold (18 K) dust in the prototypical type II supernova remnant Cassiopeia A was recently reported. It was concluded that dust production in type II supernovae can explain how the large quantities (10^8 solar masses) of dust observed in the most distant quasars could have been produced within only 700 million years after the Big Bang. Foreground clouds of interstellar material, however, complicate the interpretation of the earlier submillimetre observations of Cas A. Here we report far-infrared and molecular line observations that demonstrate that most of the detected submillimetre emission originates from interstellar dust in a molecular cloud complex located in the line of sight between the Earth and Cas A, and is therefore not associated with the remnant. The argument that type II supernovae produce copious amounts of dust is not supported by the case of Cas A, which previously appeared to provide the best evidence for this possibility.Comment: 13 pages, 3 figure

Bypass or Engage? Explaining Donor Delivery Tactics

Abstract The conventional wisdom in the literature on aid allocation suggests that donors utilize bilateral aid as a tool to buy influence in the aid-receiving country. Those who conclude that aid is driven by donor self-interest focus on government-to-government aid transfers. However, this approach overlooks important variation in delivery tactics: bilateral donors frequently provide aid to non-state actors. This paper argues that donors resort to delivery tactics that increase the likelihood of aid achieving its intended outcome. In poorly governed recipient countries, donors bypass recipient governments and deliver more aid through non-state actors, all else equal. In recipient countries with higher governance quality, donors engage the government and give more aid through the government-to-government channel. Using OLS and Probit regressions, I find empirical support for this argument. Understanding the determinants of donor delivery tactics has important implications for assessing aid effectiveness

Essential Role of Gab1 for Signaling by the C-Met Receptor in Vivo

The docking protein Gab1 binds phosphorylated c-Met receptor tyrosine kinase directly and mediates signals of c-Met in cell culture. Gab1 is phosphorylated by c-Met and by other receptor and nonreceptor tyrosine kinases. Here, we report the functional analysis of Gab1 by targeted mutagenesis in the mouse, and compare the phenotypes of the Gab1 and c-Met mutations. Gab1 is essential for several steps in development: migration of myogenic precursor cells into the limb anlage is impaired in Gab1−/− embryos. As a consequence, extensor muscle groups of the forelimbs are virtually absent, and the flexor muscles reach less far. Fewer hindlimb muscles exist, which are smaller and disorganized. Muscles in the diaphragm, which also originate from migratory precursors, are missing. Moreover, Gab1−/− embryos die in a broad time window between E13.5 and E18.5, and display reduced liver size and placental defects. The labyrinth layer, but not the spongiotrophoblast layer, of the placenta is severely reduced, resulting in impaired communication between maternal and fetal circulation. Thus, extensive similarities between the phenotypes of c-Met and HGF/SF mutant mice exist, and the muscle migration phenotype is even more pronounced in Gab1−/−:c-Met+/− embryos. This is genetic evidence that Gab1 is essential for c-Met signaling in vivo. Analogy exists to signal transmission by insulin receptors, which require IRS1 and IRS2 as specific docking proteins

Die Sieben Todsünden

Weshalb faszinieren und inspirieren die Sieben Todsünden bis heute – auch und gerade obwohl theologische Kommentare längst an Verbindlichkeit eingebüßt haben? In exemplarischen Studien widmet sich der Sammelband der Wirkungsgeschichte der Sieben Todsünden in den unterschiedlichen Künsten: Literatur und bildende Kunst, Film und Fernsehen. Der Fokus liegt weniger auf einer Ideengeschichte der Todsünden als auf deren Formelhaftigkeit, die gerade im Verblassen der ursprünglichen Hintergründe ihre Wirkmacht in breiter diskursiver Streuung entfaltet. Dabei reichen die vielfältigen Fortschreibungen und Transformationen weit über das frühe Mittelalter und die klassische Theologie hinaus und zeigen in der Moderne und Postmoderne verstärkt nur noch Allusionen auf die ursprünglich religiöse Ordnungsphantasie. So werden die Todsünden zu einem intermedialen Fundus für ethische und politische Reflexionen, ästhetische Transformationen und künstlerische Experimente. Der Band versammelt Studien, die sich aus literatur-, medien- und kulturwissenschaftlicher Perspektive sowohl den einzelnen Todsünden superbia, invidia, ira, acedia, avaritia, gula, luxuria als auch dem Septenar insgesamt widmen