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    61. 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=2159-02-1 -- 146.5 Кб -- 13.04.2016
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    62. 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=2165-02-1 -- 146.5 Кб -- 13.04.2016
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    63. 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=2167-02-1 -- 146.5 Кб -- 13.04.2016
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    64. 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=2173-02-1 -- 146.4 Кб -- 13.04.2016
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    65. 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=2175-02-1 -- 146.5 Кб -- 13.04.2016
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    66. 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=2183-02-1 -- 146.5 Кб -- 13.04.2016
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    67. 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=2185-02-1 -- 146.5 Кб -- 13.04.2016
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    68. 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=1839-02-1 -- 146.5 Кб -- 13.04.2016
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    69. 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=1835-02-1 -- 146.5 Кб -- 13.04.2016
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    70. 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=2190-02-1 -- 146.4 Кб -- 13.04.2016
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