... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...
... 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 ...