Mid-infrared observations of the transitional disks around DH Tau, DM Tau, and GM Aur

Aims: We present mid-infrared observations and photometry of the transitional disks around the young stellar objects DH Tau, DM Tau, and GM Aur, obtained with VISIR/VLT in N band. Our aim is to resolve the inner region and the large-scale structures of these transitional disks, carrying potential signatures of intermediate or later stages of disk evolution and ongoing planet formation. Methods: We use the simultaneously observed standard-stars as PSF reference to constrain the radial flux profiles of our target objects. Subtracting the obtained standard-star profile from the corresponding science object profile yields the flux residuals produced by the star-disk system. A detection threshold takes into account the background standard deviation and also the seeing variations during the observations to evaluate the significance of these flux residuals. On the basis of a simple model for the dust re-emission, we derive constraints on the inner radius of the dust disk. Results: We spatially resolve the transitional disk around GM Aur and determine an inner-disk hole radius of 20.5(+1.0,-0.5) AU. The circumstellar disks around DH Tau and DM Tau are not spatially resolved but we are able to constrain the inner-disk hole radius to <15.5(+9.0,-2.0) AU and <15.5(+0.5,-0.5) AU, respectively. The performed photometry yields fluxes of 178+-31 mJy for DH Tau, 56+-6 mJy for DM Tau, and 229+-14 mJy for GM Aur.Comment: Accepted for publication in Astronomy & Astrophysics. (6 pages, including 7 figures and 5 tables

Young men in love: the (re)making of heterosexual masculinities through ‘‘serious’’ relationships

In this paper I examine how young men’s experience of what they termed 'serious' relationships are contexts in which they were engaged in the processes of exploring and, in some important ways, remaking their masculine identities. I refer to data drawn from in-depth interviews with eight middle-class, white young men who are reaching the end of their studies in a Scottish secondary school and planning to enter higher education. I identify and explore aspects of the intimate relationship in which these young men contest culturally patterned discourses of gender difference and show how, in trying to resolve these differences, their sense of masculine identities is altered. I suggest that familiar gendered differences – relating to the ways that sex and love, commitment and independence and emotional expressiveness are linked to heterosexual masculinity and femininity – are three of the distinct fields of which these young men are aware and via which they engage in ‘‘gender’’ work. I argue that how this work is done, the resources employed and the meanings that are generated are independent on specific local and temporal realities of these young men lives

Young people's experiences of 'serious' romantic relationships in late adolescence: 'What is this thing called love?'

This thesis mounts an in-depth exploration of young, white, Scottish people's views and experiences of falling in love with people of the opposite sex in the context of 'serious' romantic relationships formed in their late adolescence. It is located within the sociology of emotion and engages with debates about how emotional experience is shaped and influenced by social interaction, structures, cultural discourses and resources. The principal questions considered are: What array of social-cultural influences are pertinent to understanding these young people's experiences of love and 'serious' relationships? How and in what ways are these influences perceived to be inflecting or constitutive of these young people's experiences? In what ways do these young people's experiences exceed the account made possible through the sociology of emotion and, what possibilities and opportunities are there for elaborating this account? The study draws principally on data generated through interviews with young people studying for Highers in the sixth year of a secondary school. A grounded approach was used in analysis of these data. Findings include the development of taxonomies of 'serious' relationships which describe their constitutive elements, address the issue of why they are especially pertinent to young people in late adolescence and how this relates to their negotiation of specific social settings, interactions and developmental events. Gender, family and transition emerge as particular salient socio-cultural influences within these young people's accounts of their 'serious' relationships and the nature of each of these is explored in depth. I argue that the theoretical framework provided by the sociology of emotion has good explicative power in terms of identifying the array of social factors which are likely to be influencing emotional experiences but there is scope both for further research and to employ additional theoretical resources, especially psycho-dynamically inflected thinking, in order to explain emotional experience at the level of individual

Lucky Imaging Adaptive Optics of the brown dwarf binary GJ569Bab

The potential of combining Adaptive Optics (AO) and Lucky Imaging (LI) to achieve high precision astrometry and differential photometry in the optical is investigated by conducting observations of the close 0\farcs1 brown dwarf binary GJ569Bab. We took 50000 $I$-band images with our LI instrument FastCam attached to NAOMI, the 4.2-m William Herschel Telescope (WHT) AO facility. In order to extract the most of the astrometry and photometry of the GJ569Bab system we have resorted to a PSF fitting technique using the primary star GJ569A as a suitable PSF reference which exhibits an $I$-band magnitude of $7.78\pm0.03$. The AO+LI observations at WHT were able to resolve the binary system GJ569Bab located at 4\farcs 92 \pm 0\farcs05 from GJ569A. We measure a separation of $98.4 \pm 1.1$ mas and $I$-band magnitudes of $13.86 \pm 0.03$ and $14.48 \pm 0.03$ and $I-J$ colors of 2.72$\pm$0.08 and 2.83$\pm$0.08 for the Ba and Bb components, respectively. Our study rules out the presence of any other companion to GJ569A down to magnitude I$\sim$ 17 at distances larger than 1\arcsec. The $I-J$ colors measured are consistent with M8.5-M9 spectral types for the Ba and Bb components. The available dynamical, photometric and spectroscopic data are consistent with a binary system with Ba being slightly (10-20%) more massive than Bb. We obtain new orbital parameters which are in good agreement with those in the literature.Comment: 13 pages, 9 figures, 7 tables, in press in MNRA

The first ten years: Aboriginal enclaves tenth anniversary

An enclave is the territory of a minority group found contained within the territory of a larger group. When the first enclave was started at Mount Lawley College in 1976, it was seen as a place where Aboriginal students could retreat from the hustle and bustle of College life to be with people they felt comfortable with, and refresh themselves for return to the wider world again. A second enclave was established at the Nedlands Campus in 1982, an external one at Broome in 1983 and in 1985 new enclaves have been established at Churchlands, Claremont and Carnarvon. In 1986 an enclave at the new Bunbury Institute of Advanced Education commenced operation. Also 1986 is the year for the establishment of a new off campus centre to commence in 1987 at Kununurra. Within the enclave students get support from each other and from staff; have a place to work on assignments or take tutorials with their personal tutor, and have facilities for making tea and coffee etc. As they become confident about aspects of college life which might at first have seemed strange or intimidating, most students involve themselves fully in all aspects of college life, mixing with non-Aboriginal students and using college facilities in the same way as other students. The enclave facilities are available throughout the length of a student\u27s course. By the end of the first year all students are expected to have gained experience and confidence in relation to college and student life. Consequently, enclave staff services tend to concentrate on each year\u27s new intake of students..

Resolved 24.5 micron emission from massive young stellar objects

Massive young stellar objects (MYSO) are surrounded by massive dusty envelopes. Our aim is to establish their density structure on scales of ~1000 AU, i.e. a factor 10 increase in angular resolution compared to similar studies performed in the (sub)mm. We have obtained diffraction-limited (0.6") 24.5 micron images of 14 well-known massive star formation regions with Subaru/COMICS. The images reveal the presence of discrete MYSO sources which are resolved on arcsecond scales. For many sources, radiative transfer models are capable of satisfactorily reproducing the observations. They are described by density powerlaw distributions (n(r) ~ r^(-p)) with p = 1.0 +/-0.25. Such distributions are shallower than those found on larger scales probed with single-dish (sub)mm studies. Other sources have density laws that are shallower/steeper than p = 1.0 and there is evidence that these MYSOs are viewed near edge-on or near face-on, respectively. The images also reveal a diffuse component tracing somewhat larger scale structures, particularly visible in the regions S140, AFGL 2136, IRAS 20126+4104, Mon R2, and Cep A. We thus find a flattening of the MYSO envelope density law going from ~10 000 AU down to scales of ~1000 AU. We propose that this may be evidence of rotational support of the envelope (abridged).Comment: 21 pages, accepted for A&

From discs to planetesimals I: evolution of gas and dust discs

I review the processes that shape the evolution of protoplanetary discs around young, solar-mass stars. I first discuss observations of protoplanetary discs, and note in particular the constraints these observations place on models of disc evolution. The processes that affect the evolution of gas discs are then discussed, with the focus in particular on viscous accretion and photoevaporation, and recent models which combine the two. I then discuss the dynamics and growth of dust grains in discs, considering models of grain growth, the gas-grain interaction and planetesimal formation, and review recent research in this area. Lastly, I consider the so-called "transitional" discs, which are thought to be observed during disc dispersal. Recent observations and models of these systems are reviewed, and prospects for using statistical surveys to distinguish between the various proposed models are discussed.Comment: 28 pages, 9 figures. Refereed review chapter for proceedings of VLTI summer school on "Circumstellar discs and planets at very high angular resolution", to appear in New Astronomy Reviews. See http://www.vlti.org/ for more detail

Genome-wide associations of gene expression variation in humans

The exploration of quantitative variation in human populations has become one of the major priorities for medical genetics. The successful identification of variants that contribute to complex traits is highly dependent on reliable assays and genetic maps. We have performed a genome-wide quantitative trait analysis of 630 genes in 60 unrelated Utah residents with ancestry from Northern and Western Europe using the publicly available phase I data of the International HapMap project. The genes are located in regions of the human genome with elevated functional annotation and disease interest including the ENCODE regions spanning 1% of the genome, Chromosome 21 and Chromosome 20q12-13.2. We apply three different methods of multiple test correction, including Bonferroni, false discovery rate, and permutations. For the 374 expressed genes, we find many regions with statistically significant association of single nucleotide polymorphisms (SNPs) with expression variation in lymphoblastoid cell lines after correcting for multiple tests. Based on our analyses, the signal proximal (cis-) to the genes of interest is more abundant and more stable than distal and trans across statistical methodologies. Our results suggest that regulatory polymorphism is widespread in the human genome and show that the 5-kb (phase I) HapMap has sufficient density to enable linkage disequilibrium mapping in humans. Such studies will significantly enhance our ability to annotate the non-coding part of the genome and interpret functional variation. In addition, we demonstrate that the HapMap cell lines themselves may serve as a useful resource for quantitative measurements at the cellular level

High-throughput analysis of candidate imprinted genes and allele-specific gene expression in the human term placenta.

BACKGROUND: Imprinted genes show expression from one parental allele only and are important for development and behaviour. This extreme mode of allelic imbalance has been described for approximately 56 human genes. Imprinting status is often disrupted in cancer and dysmorphic syndromes. More subtle variation of gene expression, that is not parent-of-origin specific, termed 'allele-specific gene expression' (ASE) is more common and may give rise to milder phenotypic differences. Using two allele-specific high-throughput technologies alongside bioinformatics predictions, normal term human placenta was screened to find new imprinted genes and to ascertain the extent of ASE in this tissue. RESULTS: Twenty-three family trios of placental cDNA, placental genomic DNA (gDNA) and gDNA from both parents were tested for 130 candidate genes with the Sequenom MassArray system. Six genes were found differentially expressed but none imprinted. The Illumina ASE BeadArray platform was then used to test 1536 SNPs in 932 genes. The array was enriched for the human orthologues of 124 mouse candidate genes from bioinformatics predictions and 10 human candidate imprinted genes from EST database mining. After quality control pruning, a total of 261 informative SNPs (214 genes) remained for analysis. Imprinting with maternal expression was demonstrated for the lymphocyte imprinted gene ZNF331 in human placenta. Two potential differentially methylated regions (DMRs) were found in the vicinity of ZNF331. None of the bioinformatically predicted candidates tested showed imprinting except for a skewed allelic expression in a parent-specific manner observed for PHACTR2, a neighbour of the imprinted PLAGL1 gene. ASE was detected for two or more individuals in 39 candidate genes (18%). CONCLUSIONS: Both Sequenom and Illumina assays were sensitive enough to study imprinting and strong allelic bias. Previous bioinformatics approaches were not predictive of new imprinted genes in the human term placenta. ZNF331 is imprinted in human term placenta and might be a new ubiquitously imprinted gene, part of a primate-specific locus. Demonstration of partial imprinting of PHACTR2 calls for re-evaluation of the allelic pattern of expression for the PHACTR2-PLAGL1 locus. ASE was common in human term placenta.RIGHTS : This article is licensed under the BioMed Central licence at http://www.biomedcentral.com/about/license which is similar to the 'Creative Commons Attribution Licence'. In brief you may : copy, distribute, and display the work; make derivative works; or make commercial use of the work - under the following conditions: the original author must be given credit; for any reuse or distribution, it must be made clear to others what the license terms of this work are