... fragment into massive clumps, at least some of which will undergo further collapse and end up as massivestars/clusters ... Evidence of active massivestar formation is detected towards at least one clump of the dust-ring of G351.77-0.54, while ...
... Gemini Core Science . Brown Dwarfs and Low MassStars . Young Star Clusters . YSO Jet Driving Mechanism . ... Recent near-infrared sky surveys have succeeded in identifying large numbers of low massstars and brown dwarfs. ...
... diagram the pathways of stars of 1, 5 and 10 solar masses during their life cycle ... Post-Main Sequence . Solar MassStar Death . High MassStar Death . Star Clusters . ...
... Hot Molecular Core'? ~104 yr Molecular Cold Core Cloud Hot Core Phase Methanol Maser ~105 yr UCHII Phase MassiveStar ~104 yr ... J(1-0), =89.189 GHz · Exhibits saturated and self-absorbed line profiles in regions of massivestar-formation. ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/mm_science2002/talks/cpurcell.pdf -- 514.7 Кб -- 26.11.2002 Похожие документы
... Observations of other massivestar regions ~10%(Alecian & MiMes collaboration). ... exhibits a highly abnormal massive-starmass function (Pflamm-Altenburg & Kroupa ...
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Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/ferrario.pdf -- 1130.3 Кб -- 16.06.2010 Похожие документы
... Planetary nebulae are the remnants of low-to-middle massstars. ... layers of gas have blown away, stars change from losing mass in slow dense winds to ... These are thought to be unusually massivestars and the precursors to the more ...
... 4th of April 2016 . Do massive binary stars emit -rays ? . by Paula Benaglia (IAR UNLP) . ... Compelling evidence that massive binary stars are -ray emitters was found only for the strange system Eta Carina ( Abdo et al. ...
... much has been learnt about how low-massstars (i.e. solar mass and below) form in ... II clouds, two nearby clouds where low massstar formation occurs, but with quite ...
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Ссылки http://www.atnf.csiro.au/management/atuc/2004jun/docs/3.1c2_DeltaQuadrant.doc -- 114.0 Кб -- 07.06.2004 Похожие документы