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Timing neutron stars = pulsations, o...

Belloni, Tomaso M.

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Timing neutron stars = pulsations, oscillations and explosions /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Timing neutron stars/ edited 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.
[NT 15003449]:	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.
Contained By:	Springer Nature eBook
Subject:	Neutron stars. -
Online resource:	https://doi.org/10.1007/978-3-662-62110-3
ISBN:	9783662621103

Timing neutron stars = pulsations, 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 ;v.461..

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:

706876
Neutron stars.

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

Dewey Class. No.: 523.8874

Timing neutron stars = pulsations, oscillations and explosions /
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245 0 0 $a Timing neutron stars $h [electronic resource] : $b pulsations, oscillations and explosions / $c edited by Tomaso M. Belloni, Mariano Mendez, Chengmin Zhang.
260 $a Berlin, Heidelberg : $b Springer Berlin Heidelberg : $b Imprint: Springer, $c 2021.
300 $a xii, 335 p. : $b ill., digital ; $c 24 cm.
490 1 $a Astrophysics and space science library, $x 0067-0057 ; $v v.461
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.
650 0 $a Neutron stars. $3 706876
650 1 4 $a Astronomy, Astrophysics and Cosmology. $3 890823
700 1 $a Belloni, Tomaso M. $3 3487211
700 1 $a Mendez, Mariano. $3 3487212
700 1 $a Zhang, Chengmin. $3 3487213
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773 0 $t Springer Nature eBook
830 0 $a Astrophysics and space science library ; $v v.461. $3 3487214
856 4 0 $u https://doi.org/10.1007/978-3-662-62110-3
950 $a Physics and Astronomy (SpringerNature-11651)