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Timing neutron starspulsations, osci...

Belloni, Tomaso M.

Timing neutron starspulsations, oscillations and explosions /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Timing neutron starsedited by Tomaso M. Belloni, Mariano Mendez, Chengmin Zhang.
Reminder of title:	pulsations, oscillations and explosions /
other author:	Belloni, Tomaso M.
Published:	Berlin, Heidelberg :Springer Berlin Heidelberg :2021.
Description:	xii, 335 p. :ill., digital ;24 cm.
Contained By:	Springer Nature eBook
Subject:	Neutron stars.
Online resource:	https://doi.org/10.1007/978-3-662-62110-3
ISBN:	9783662621103$q(electronic bk.)

Timing neutron starspulsations, oscillations and explosions /
Timing neutron starspulsations, oscillations and explosions /[electronic resource] :edited by Tomaso M. Belloni, Mariano Mendez, Chengmin Zhang. - Berlin, Heidelberg :Springer Berlin Heidelberg :2021. - xii, 335 p. :ill., digital ;24 cm. - Astrophysics and space science library,v.4610067-0057 ;. - Astrophysics and space science library ;379..

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$q(electronic bk.)

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

339855
Neutron stars.

LC Class. No.: QB843.N4 / T55 2021

Dewey Class. No.: 523.8874

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505 0 $a 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.
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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