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    11. Terms and Definitions
    ... rock thrown out of the crater during its formation that either falls back to partly fill the crater or blankets its outer ... associated with craters; Pamlimpsests are thought to be impact craters where the topographic relief of the crater has been ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/terms.htm -- 45.4 Кб -- 15.03.1998
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    12. APOD: 2000 July 13 - LP 944-20: A Failed Star Flares
    ... star recently startled astronomers by producing a flare visible at x-ray energies ... The above Chandra X-ray Observatory images of the LP944-20 star field were recorded ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/lp944-20_cxo.html -- 5.0 Кб -- 25.01.2001
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    13. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1849-02-1 -- 146.5 Кб -- 13.04.2016
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    14. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1851-02-1 -- 146.5 Кб -- 13.04.2016
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    15. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1862-02-1 -- 146.5 Кб -- 13.04.2016
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    16. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1857-02-1 -- 146.5 Кб -- 13.04.2016
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    17. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1861-02-1 -- 146.5 Кб -- 13.04.2016
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    18. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1837-02-1 -- 146.5 Кб -- 13.04.2016
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    19. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1855-02-1 -- 146.5 Кб -- 13.04.2016
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    20. INAF - Osservatorio di Arcetri
    ... a natural explanation for two observed trends in aged pulsar wind nebulae (PWNe): a steady increase of the PWN X-ray size with its age, up to ages of about 10^5 yr, and a rather narrow correlation between pulsar spin down power and PWN X-ray luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/index.php?option=com_content&view=category&Itemid=424&id=202&iccaldate=1858-02-1 -- 146.4 Кб -- 13.04.2016
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