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    1. P Cygni 2000 Workshop
    ... The middle structure, originally called the Integral Nebula, is an emission nebula, seen in hundreds of emission lines throughout the visible and near-ultraviolet portion of the spectrum. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/archive/pcyg2000.html -- 41.5 Кб -- 29.11.2001
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    2. M.D. Smith, Research Astronomer
    ... Figure 8: The appearance of a variable nebula at various epochs in the optical I-band, atomic [S II ] and near-infrared K-band emission, probably illuminated by radiation from an outbursting protostar. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2003/node62.html -- 10.8 Кб -- 19.05.2004
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    3. http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-8-pulsars-and-final-overview.pdf
    ... is slowing down by radiating lowfrequency EM waves Leverhulme Lectures on Stellar Magnetism 07/05/09 Rotationally powered emission region in Crab Nebula Composite image of supernova remnant from SN 1054 explosion Pulsar is blue star at centre, powering EM ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-8-pulsars-and-final-overview.pdf -- 688.4 Кб -- 05.07.2009
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    4. Armagh Observatory PhD Theses
    ... E.M. Lindsay . 1971 . Flare Stars in the Orion Nebula . David Andrews . T. Kiang . ... 2007 . Properties of the Radio Emission at the Stellar/Substellar Boundary . ... Radio Emission from Ultracool Dwarfs and . the Relevant Radiation Mechanisms . ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/PhD-Thesis/thesis.html -- 14.2 Кб -- 01.09.2014
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    5. http://star.arm.ac.uk/~ambn/261mzb.ps
    ... Therefore the origin of the emission lies in a nebula which not necessarily surrounds the star but may be in the foreground or in the background; there is no reason to believe that the emission is taking place in any circumstellar material. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/261mzb.ps -- 432.8 Кб -- 11.02.1997
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    6. Armagh Observatory
    ... Extinction, emission, linear and circular polarisation. ... wavelength-dependence of extinction, emission, linear and circular polarisation of ... We tabulate parameters for PAH emission bands in various environments. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2013/639.html -- 6.7 Кб -- 09.09.2013
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    7. Sakurai?s Object (V4334 Sagittarii)
    ... When it failed to show any hydrogen emissions from the star, the charateristic of a nova, they realised that this was a very ... It was then discovered that Sakaurai?s object has a faint planetary nebula surrounding the star. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/essays/Sakurai.htm -- 8.9 Кб -- 01.10.2012
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    8. http://star.arm.ac.uk/preprints/2013/639.pdf
    ... The dust emission between 5 ­ 35 µm in the northern part of the nebula is modelled ... it might be dominated by cold dust emission of the molecular cloud behind the nebula ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2013/639.pdf -- 794.6 Кб -- 09.09.2013
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    9. Armagh Observatory
    ... The scatter is thought to be due to a combination of uncertainty and natural H emission variability. Abstract . ... 587 known low-mass members of the star-forming region NGC2264 (Cone Nebula), arriving at a median age of 3.0 Myr, an accretion ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2012/627.html -- 6.4 Кб -- 28.11.2012
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    10. http://star.arm.ac.uk/~csj/papers/newsletter/ccp7n21_jeffery2.ps
    ... Whilst these are also central stars of low­excitation PN, the stellar emission spectrum is quite distinct form that of the nebula. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/newsletter/ccp7n21_jeffery2.ps -- 168.0 Кб -- 30.10.2001
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