48 research outputs found

    A Triple Protostar System Formed via Fragmentation of a Gravitationally Unstable Disk

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    Binary and multiple star systems are a frequent outcome of the star formation process, and as a result, almost half of all sun-like stars have at least one companion star. Theoretical studies indicate that there are two main pathways that can operate concurrently to form binary/multiple star systems: large scale fragmentation of turbulent gas cores and filaments or smaller scale fragmentation of a massive protostellar disk due to gravitational instability. Observational evidence for turbulent fragmentation on scales of >>1000~AU has recently emerged. Previous evidence for disk fragmentation was limited to inferences based on the separations of more-evolved pre-main sequence and protostellar multiple systems. The triple protostar system L1448 IRS3B is an ideal candidate to search for evidence of disk fragmentation. L1448 IRS3B is in an early phase of the star formation process, likely less than 150,000 years in age, and all protostars in the system are separated by <<200~AU. Here we report observations of dust and molecular gas emission that reveal a disk with spiral structure surrounding the three protostars. Two protostars near the center of the disk are separated by 61 AU, and a tertiary protostar is coincident with a spiral arm in the outer disk at a 183 AU separation. The inferred mass of the central pair of protostellar objects is \sim1 Msun_{sun}, while the disk surrounding the three protostars has a total mass of \sim0.30 M_{\sun}. The tertiary protostar itself has a minimum mass of \sim0.085 Msun_{sun}. We demonstrate that the disk around L1448 IRS3B appears susceptible to disk fragmentation at radii between 150~AU and 320~AU, overlapping with the location of the tertiary protostar. This is consistent with models for a protostellar disk that has recently undergone gravitational instability, spawning one or two companion stars.Comment: Published in Nature on Oct. 27th. 24 pages, 8 figure

    Land management impacts on European butterflies of conservation concern: a review

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    Child behaviour after anaesthesia: association of socioeconomic factors and child behaviour checklist to the Post-Hospital Behaviour Questionnaire

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    AIM: In the process of validation of the Swedish translation of the Post-Hospital Behaviour Questionnaire (PHBQ) to assess its relation to the Child Behaviour Checklist (CBCL) and to describe its relation to sociodemographic factors. METHOD: Three hundred and forty children 2-13 years studied in connection with elective procedures which included anaesthesia. Parents completed the CBCL forms before and after hospitalization as well as the PHBQ 2 weeks after hospitalization. RESULTS: In multivariate analysis of PHBQ total score independent risk factors were: age &lt;5 (OR 2.4; CI 1.4-4.0), living in a one parent family (OR 4.4; CI: 1.6-12.6) and not living in a rural area (OR 1.6; CI: 1.0-2.6). The correlation between the total scores for PHBQ and CBCL for children aged 2-4 was moderate: (r = 0.38; p &lt; 0.005). For children aged 4-7 there were significant correlations between PHBQ sleep anxiety and CBCL Other problems (r = 0.4; p &lt; 0.01), PHBQ eating disturbances and CBCL total score (r = 0.3; p &lt; 0.01), though none of these significant correlations were observed for children above 7 years of age. CONCLUSION: There is an association between PHBQ and CBCL which is weaker for older children. The reason for this might be that PHBQ is more sensitive in the younger age group and to minor changes in behaviour. Children younger than 5 years of age or living in a one parent family or not living in rural areas appear to have higher incidence of problematic behaviour in a 2 week follow up after anaesthesia.Karling, M Hagglof, B Research Support, Non-U.S. Gov't Norway Acta paediatrica (Oslo, Norway : 1992) Acta Paediatr. 2007 Mar;96(3):418-23
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