2,388 research outputs found

    The colour-magnitude relation of Globular Clusters in Centaurus and Hydra - Constraints on star cluster self-enrichment with a link to massive Milky Way GCs

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    We investigate the colour-magnitude relation of metal-poor globular clusters, the 'blue tilt', in the Hydra and Centaurus galaxy clusters and constrain the primordial conditions for star cluster self-enrichment. We analyse U,I photometry for about 2500 globular clusters in the central regions of Hydra and Centaurus, based on FORS1@VLT data. We convert the measured colour-magnitude relations into mass-metallicity space and obtain a scaling of Z \propto M^{0.27 \pm 0.05} for Centaurus GCs and Z \propto M^{0.40 \pm 0.06} for Hydra GCs, consistent with results in other environments. We find that the GC mass-metallicity relation already sets in at present-day masses of a few 10^5 solar masses and is well established in the luminosity range of massive MW clusters like omega Centauri. We compare the mass-metallicity relation with predictions from the star cluster self-enrichment model by Bailin & Harris (2009). For this we include effects of dynamical and stellar evolution and a physically well motivated primordial mass-radius scaling. The self-enrichment model reproduces the observed relations well for average primordial half-light radii r_h ~ 1-1.5 pc, star formation efficiencies f_* ~ 0.3-0.4, and pre-enrichment levels of [Fe/H] ~ -1.7 dex. Within the self-enrichment scenario, the observed blue tilt implies a correlation between GC mass and width of the stellar metallicity distribution. We find that this implied correlation matches the trend of width with GC mass measured in Galactic GCs, including extreme cases like omega Cen and M54. We conclude that 1. A primordial star cluster mass-radius relation provides a significant improvement to the self-enrichment model fits. 2. Broadenend metallicity distributions as found in some massive MW globular clusters may have arisen naturally from self-enrichment processes, without the need of a dwarf galaxy progenitor.Comment: 15 pages, 13 figures. Language edited version of paper accepted for publication in Astronomy & Astrophysics. Colour-composite in Figure 1 reduced in resolutio

    Long-Term Spiritual Growth and its Influence on Professional Endeavor

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    This paper presents a qualitative study of how long-term practitioners of Integral Yoga working in four fields of professional endeavour—business management, education, health care, and the arts—have applied Integral Yoga in their work and how they perceived its influences. The paper gives a brief overview of the nature of Integral Yoga, especially its aspect of karmayoga, and an explanation of the study’s method which involved semi-structured interviews with 12 residents or regular visitors to the Sri Aurobindo Ashram or Auroville. Ten common themes were identified which emerged in at least three of the interviews and in at least two fields of work. The report of the findings focuses on the participants’ lived experiences of Integral Yoga and its perceived effects in their various fields of work

    INDIVIDUALISM AND ECONOMIC ORDER. By Frederich A. Hayek. Chicago. University of Chicago Press, 1948

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    A megahertz active pixel sensor for X-ray astronomy

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    A megahertz active pixel sensor for X-ray astronomy

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    Zeichnungen alter deutscher Meister in Dessau

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