11,971 research outputs found

    The [alpha/Fe] Ratios in Dwarf Galaxies: Evidence for a Non-universal Stellar Initial Mass Function?

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    It is well established that the [alpha/Fe] ratios in elliptical galaxies increase with galaxy mass. This relation holds also for early-type dwarf galaxies, although it seems to steepen at low masses. The [alpha/Fe] vs. mass relation can be explained assuming that smaller galaxies form over longer timescales (downsizing), allowing a larger amount of Fe (mostly produced by long-living Type Ia Supernovae) to be released and incorporated into newly forming stars. Another way to obtain the same result is by using a flatter initial mass function (IMF) in large galaxies, increasing in this way the number of Type II Supernovae and therefore the production rate of alpha-elements. The integrated galactic initial mass function (IGIMF) theory predicts that the higher the star formation rate, the flatter the IMF. We have checked, by means of semi-analytical calculations, that the IGIMF theory, combined with the downsizing effect (i.e. the shorter duration of the star formation in larger galaxies), well reproduces the observed [alpha/Fe] vs. mass relation. In particular, we show a steepening of this relation in dwarf galaxies, in accordance with the available observations.Comment: 4 pages, 2 figures; to appear in the proceedings of the JENAM 2010 Symposium on Dwarf Galaxies (Lisbon, September 9-10, 2010

    Learning how much about gases using MBL? A case study from a chemistry classroom

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    Chemistry learning with understanding is a challenge. From a social constructivist position we view students ‘chemistry learning from experiments as involving the shared negotiation of meaning that uses experimental data to confirm or challenge their existing scientific theories. This study investigated teaching and learning practices related to the use of MBL in a high school chemistry laboratory where students were studying gases and kinetic theory. Given the widely accepted view that the use of such technology is a ‘cure-all’ for educational problems, the learning of students as a consequence of their use of this technology might be considered disappointing. We find that little or no higher order thinking was employed as students engaged in using the MBL and that some alternative conceptions remained unchallenged through its use. It is necessary to consider the positioning of the computer in the group and experimental context if the promise of the use of such technology is to be fulfilled.published_or_final_versio

    And the winner is: galaxy mass

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    The environment is known to affect the formation and evolution of galaxies considerably best visible through the well-known morphology-density relationship. We study the effect of environment on the evolution of early-type galaxies for a sample of 3,360 galaxies morphologically selected by visual inspection from the SDSS in the redshift range 0.05<z<0.06, and analyse luminosity-weighted age, metallicity, and alpha/Fe ratio as function of environment and galaxy mass. We find that on average 10 per cent of early-type galaxies are rejuvenated through minor recent star formation. This fraction increases with both decreasing galaxy mass and decreasing environmental density. However, the bulk of the population obeys a well-defined scaling of age, metallicity, and alpha/Fe ratio with galaxy mass that is independent of environment. Our results contribute to the growing evidence in the recent literature that galaxy mass is the major driver of galaxy formation. Even the morphology-density relationship may actually be mass-driven, as the consequence of an environment dependent characteristic galaxy mass coupled with the fact that late-type galaxy morphologies are more prevalent in low-mass galaxies.Comment: 5 pages, proceedings of JENAM 2010, Symposium 2: "Environment and the formation of galaxies: 30 years later

    UNDERSTANDING FIBROIDS IN LIGHT OF AYURVEDA

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    The changing lifestyle and dietary pattern has given way to many gynecological problems in females. Uterine fibroids are one of leading concerns for women in reproductive age. Though uterine fibroids are non- cancerous in character; they exhibit a wide range of symptoms like dysmenorrhea, menorrhagia, metrorrhagia, low backache etc. It significantly hampers the general health and quality of life in women causing great mental agony. Contemporary treatment protocols include hormonal therapy, hysterectomy, myomectomy and uterine artery embolization. Reluctance to undergo prolonged hormone therapy, the fear of surgery brings more and more patient to Ayurveda. Hence more systematic studies in conservative management in these areas of Stree Roga are need of the hour. Ayurveda classics mention various pathological conditions that have features similar to fibroids. Owing to its muscular origin, with slow growth may be better compared to Granthi in Garbhasya. In the modern era of busy lifestyle, intake of junk food, lack of exercise etc had lead to Agnivaishamya and Ama formation. This in turn vitiates Doshas like Kapha and Vata and Dushyas like Rasa, Raktha, Mamsa, Medas and Arthava resulting in Dhatwagnimandya leading to formation of Garbhasayagranthi. The treatment approach is directed towards reducing size of fibroids using Ushna, Tiskhna, Lekhana Dravyas along with management of symptoms. The inevitable roles of Vata in Yoniroga is also taken into account in its management. Combining different treatment aspects of Granthi and Yoni Roga Chitksa, a unique approach towards the management of its varied presentations added on with lifestyle modification can contribute to healthy social life. The current article focuses and explores potentials of Ayurveda in different aspects of uterine fibroid

    Quality ratings of frequency-compressed speech by participants with extensive high-frequency dead regions in the cochlea.

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    OBJECTIVE: The objective was to assess the degradation of speech sound quality produced by frequency compression for listeners with extensive high-frequency dead regions (DRs). DESIGN: Quality ratings were obtained using values of the starting frequency (Sf) of the frequency compression both below and above the estimated edge frequency, fe, of each DR. Thus, the value of Sf often fell below the lowest value currently used in clinical practice. Several compression ratios were used for each value of Sf. Stimuli were sentences processed via a prototype hearing aid based on Phonak Exélia Art P. STUDY SAMPLE: Five participants (eight ears) with extensive high-frequency DRs were tested. RESULTS: Reductions of sound-quality produced by frequency compression were small to moderate. Ratings decreased significantly with decreasing Sf and increasing CR. The mean ratings were lowest for the lowest Sf and highest CR. Ratings varied across participants, with one participant rating frequency compression lower than no frequency compression even when Sf was above fe. CONCLUSIONS: Frequency compression degraded sound quality somewhat for this small group of participants with extensive high-frequency DRs. The degradation was greater for lower values of Sf relative to fe, and for greater values of CR. Results varied across participants.Action on Hearing Loss, Phonak AG, H.B. Allen Trust, Medical Research CouncilThis is the final version of the article. It first appeared from Taylor & Francis via http://dx.doi.org/10.1080/14992027.2016.123407

    Potent and selective inhibitors of histone deacetylase-3 containing chiral oxazoline capping groups and a N-(2-Aminophenyl)-benzamide binding unit

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    A novel series of potent chiral inhibitors of histone deacetylase (HDAC) is described that contains an oxazoline capping group and a N-(2-aminophenyl)-benzamide unit. Among several new inhibitors of this type exhibiting Class I selectivity and potent inhibition of HDAC3-NCoR2, in vitro assays for the inhibition of HDAC1, HDAC2, and HDAC3-NCoR2 by N-(2-aminophenyl)-benzamide 15k gave respective IC50 values of 80, 110, and 6 nM. Weak inhibition of all other HDAC isoforms (HDAC4, 5, 6, 7, and 9: IC50 > 100 000 nM; HDAC8: IC50 = 25 000 nM; HDAC10: IC50 > 4000 nM; HDAC11: IC50 > 2000 nM) confirmed the Class I selectivity of 15k. 2-Aminoimidazolinyl, 2-thioimidazolinyl, and 2-aminooxazolinyl units were shown to be effective replacements for the pyrimidine ring present in many other 2-(aminophenyl)-benzamides previously reported, but the 2-aminooxazolinyl unit was the most potent in inhibiting HDAC3-NCoR2. Many of the new HDAC inhibitors showed higher solubilities and lower binding to human serum albumin than that of Mocetinostat. Increases in histone H3K9 acetylation in the human cell lines U937 and PC-3 was observed for all three oxazolinyl inhibitors evaluated; those HDAC inhibitors also lowered cyclin E expression in U937 cells but not in PC-3 cells, indicating underlying differences in the mechanisms of action of the inhibitors on those two cell lines

    Decadal-scale onset and termination of Antarctic ice-mass loss during the last deglaciation.

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    Emerging ice-sheet modeling suggests once initiated, retreat of the Antarctic Ice Sheet (AIS) can continue for centuries. Unfortunately, the short observational record cannot resolve the tipping points, rate of change, and timescale of responses. Iceberg-rafted debris data from Iceberg Alley identify eight retreat phases after the Last Glacial Maximum that each destabilized the AIS within a decade, contributing to global sea-level rise for centuries to a millennium, which subsequently re-stabilized equally rapidly. This dynamic response of the AIS is supported by (i) a West Antarctic blue ice record of ice-elevation drawdown >600 m during three such retreat events related to globally recognized deglacial meltwater pulses, (ii) step-wise retreat up to 400 km across the Ross Sea shelf, (iii) independent ice sheet modeling, and (iv) tipping point analysis. Our findings are consistent with a growing body of evidence suggesting the recent acceleration of AIS mass loss may mark the beginning of a prolonged period of ice sheet retreat and substantial global sea level rise
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