'Millisecond pulsar' diaporamas de présentation

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1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun , radius i

Final States of a Star. 1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun , radius is about that of the Earth) 2. Neutron Star If initial mass > 8 M Sun and < 25 M Sun . 3. Black Hole

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The Planets of Other Stars

The Planets of Other Stars The Astronomy Diagnostic Test (ADT): The Sequel On the first day of class, the University requested that everyone fill out an online questionnaire through Angel . Now they want you to do it again.

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The Planets of Other Stars

The Planets of Other Stars. The Astronomy Diagnostic Test (ADT): The Sequel. On the first day of class, the University requested that everyone fill out an online questionnaire through Angel . Now they want you to do it again.

367 views • 25 slides

ACCRETING X-RAY MILLISECOND PULSARS

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Evolution of X-ray Binaries and the Formation of Binary Pulsars

Evolution of X-ray Binaries and the Formation of Binary Pulsars. Xiang-Dong Li Department of Astronomy Nanjing University. Millisecond Pulsar (MSP)-X-ray Binary (XRB) Relation. ATNF PSR Database. Spin Frequency Distribution in LMXBs. Binary Pulsar Populations. Binary Pulsar Populations.

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Giant Pulses of Pulsar Radio Emission A.D. Kuzmin Pushino Radio Astronomy Observatory

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A Plethora of Pulsars

A Plethora of Pulsars. Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration. Fermi LAT Pulsar Discoveries.

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Neutron stars in globular clusters : XMM-Newton results

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