... Cleaning up Eta Carina: Detection of Ammonia in the Homunculus Smith et al. (2006) report the first detection of ammonia in the Homunculus nebula around Carina, which is also the first d etection of emission fro m a p olyatomic molecule in this or any ...
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Ссылки http://www.atnf.csiro.au/management/atuc/2006jun/docs/4_Astrophys.pdf -- 1379.3 Кб -- 02.06.2006 Похожие документы
... The 20 m BB filter can usually only be productively used at a dry site like Mauna Kea observatory, although it was used to observe Carina at 17 m from the AAT in 1994. ...
... NGC3603 in Carina Image: http://hubblesite.org/ News Release Number: STScI-2007-34 An EvoluFonary Timeline for High Mass Star FormaFon: Parkes 50th Anniversary Occupy Wall Street Occupy Wall Street has been driven by the disproportionate fraction of ...
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Ссылки http://www.atnf.csiro.au/research/conferences/Parkes50th/SimonEllingsen.pdf -- 2473.2 Кб -- 08.11.2011 Похожие документы
... The data are consistent with a tangent point of ~49.5° for the Carina-Sagittarius spiral arm, which also explains the decrease in source numbers for l > 50° The total number of methanol masers ! ...
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Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/403_Pandian.pdf -- 1225.0 Кб -- 26.04.2007 Похожие документы
... Using the mean rotation curve of Brand and Blitz (1993) implies that these HII regions are located outside the solar circle at about 9.5 kpc from the Sun and hence are localised in the far part of the Carina arm. ...
... Canopus, н± Carinae, has an apparent magnitude of -0.62 whilst Mimosa, нІ Crucis, has an apparent magnitude of +1.25. a) Which appears brightest? . ...