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    31. http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch3.pdf
    ... to star formation (SF from here on) because generally only young, massive stars ... star formation tracers affected by dust attenuation (e.g., H, UV) show a much larger ... star forming regions dominates in the plane, the 24 µm emission has a direct ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch3.pdf -- 543.8 Кб -- 21.10.2013
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    32. Magellanic Complexes
    ... The Bridge is the only high-velocity cloud which is known to contain stars, and the age of many of the stellar concentrations (10 - 25 Myr) indicates that the Bridge is a star forming region (Grondin, Demers and Kunkel 1992). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/putman/paper/node2.html -- 57.0 Кб -- 08.04.2016
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    33. http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch7.pdf
    ... star formation tracers affected by dust attenuation (e.g., H, UV) show a much larger ... star forming regions dominates in the plane, the 24 µm emission has a direct ... star forming properties of a galaxy, a clear and obvious trend should be observed ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch7.pdf -- 143.6 Кб -- 21.10.2013
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    34. http://www.atnf.csiro.au/people/rnorris/papers/n214.pdf
    ... In an important and beautiful Morning Star Ceremony, earthly Yolngu people communicate with their ancestors living on Baralku, the island of the dead, with the help of Banumbirr together with a Morning Star Pole. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/rnorris/papers/n214.pdf -- 384.2 Кб -- 02.12.2007
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    35. ATNF Publications 2004
    ... BROWN, A., DAY, F. & WALTER, F.M. "Radio emission from young stars in the Chamaeleon and Upper Scorpius star formation regions ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/publications/AT2004.html -- 99.4 Кб -- 08.04.2016
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    36. http://www.atnf.csiro.au/pasa/15_2/storey/paper.pdf
    ... stars 1 Introduction The X-ray pulsar GX 1+4 has been identified with the symbiotic ... star, and the emission region is modelled as a thin slab of plasma on the polar cap ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_2/storey/paper.pdf -- 142.2 Кб -- 27.07.1998
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    37. http://www.atnf.csiro.au/people/Ray.Norris/papers/n237.pdf
    ... radio continuum: stars - stars: individual: CU Virginis - stars: magnetic fields - radiation mechanisms: non-thermal - stars ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n237.pdf -- 189.3 Кб -- 23.09.2010
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    38. http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf
    ... Revealing the transition from post-AGB stars to planetary nebulae: non-thermal and ... I. Opaque atomic gas and star formation rate density". ... the frying pan: a young pulsar with a long radio trail emerging from SNR G315.9-0.0 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf -- 85.2 Кб -- 03.03.2010
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    39. http://www.atnf.csiro.au/people/Ray.Norris/papers/n254.pdf
    ... unlike European constellations which are traced out by stars, the Emu is traced by the mysterious dark spaces between the stars ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n254.pdf -- 697.5 Кб -- 23.09.2010
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    40. http://www.atnf.csiro.au/the_atnf/annual_reports/2001/Chapter4.pdf
    ... Moreover, careful modelling of these data tell us that the mass loss of this pre-supernova star was 10-7 solar masses per year, typical of evolved stars. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2001/Chapter4.pdf -- 1197.6 Кб -- 18.11.2002
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