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Timing Neutron Stars: Pulsations, Oscillations and Explosions

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Timing Neutron Stars: Pulsations, Oscillations and Explosions/ edited by Tomaso M. Belloni, Mariano Méndez, Chengmin Zhang.
其他作者:	Zhang, Chengmin.
面頁冊數:	XII, 335 p. 92 illus., 58 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Astronomy, Astrophysics and Cosmology. -
電子資源:	https://doi.org/10.1007/978-3-662-62110-3
ISBN:	9783662621103

Timing Neutron Stars: Pulsations, Oscillations and Explosions
Timing Neutron Stars: Pulsations, Oscillations and Explosions[electronic resource] /edited by Tomaso M. Belloni, Mariano Méndez, Chengmin Zhang. - 1st ed. 2021. - XII, 335 p. 92 illus., 58 illus. in color.online resource. - Astrophysics and Space Science Library,4612214-7985 ;. - Astrophysics and Space Science Library,410.

1. Astrophysical Constraints on Dense Matter in Neutron Stars -- 2. General Relativity Measurements from Pulsars -- 3. Magnetars: A Short Review and Some Sparse Considerations -- 4. Accreting Millisecond X-ray Pulsars -- 5. Thermonuclear X-ray Bursts -- 6. High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries.

Neutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability.

ISBN: 9783662621103

Standard No.: 10.1007/978-3-662-62110-3doiSubjects--Topical Terms:

593936
Astronomy, Astrophysics and Cosmology.

LC Class. No.: QB1-991

Dewey Class. No.: 520

Timing Neutron Stars: Pulsations, Oscillations and Explosions
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520 $a Neutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability.
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