'Common envelope' diaporamas de présentation

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Stellar Duets: How Companions Shape the Life and Evolution of Stars Orsola De Marco

Stellar Duets: How Companions Shape the Life and Evolution of Stars Orsola De Marco American Museum of Natural History February 18 th , 2005. Merging binaries. Simulations UKAFF. The Question that drives us: How does binarity change stellar evolution?.

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Current Status of Neutron Stars: Astrophysical Point of View

HNP2011@apctp.11.2.23. Current Status of Neutron Stars: Astrophysical Point of View. Chang-Hwan Lee @. Contents. Motivation Maximum Neutron Star Mass (Observations) Formation & Evolution of NS Binaries. Motivations 1: why Neutron Stars ?.

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The Weirdest Objects in the Universe

The Weirdest Objects in the Universe. General Relativity. Premise: acceleration and gravity are equivalent ( i.e., are you accelerating or falling in a gravitational field?) Since the speed of light is always the same, this means that the path of light can be bent by gravity.

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The Elusive Nature of (early) R-stars

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Based on Two planets orbiting the recently formed post-common envelope binary NN Serpentis

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Common Envelope Evolution through Planetary Nebula Eyes Orsola De Marco

Common Envelope Evolution through Planetary Nebula Eyes Orsola De Marco American Museum of Natural History. Collaborators: H.E. Bond, M. Moe, M.-M. Mac Low, E. Sandquist, F. Herwig, R. Taam. Merging binaries. Simulations UKAFF. Outline.

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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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Magnetars origin and progenitors with enhanced rotation

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