Plasma magnetosphere formation around oscillating magnetized neutron stars

B. J. Ahmedov; V. S. Morozova

doi:10.1007/s10509-009-9978-9

Plasma magnetosphere formation around oscillating magnetized neutron stars

B. J. Ahmedov, V. S. Morozova

Physics

Research output: Contribution to journal › Article › peer-review

8 Scopus citations

Abstract

The notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission in the region of open field lines of plasma magnetosphere.

Original language	English (US)
Pages (from-to)	115-117
Number of pages	3
Journal	Astrophysics and Space Science
Volume	319
Issue number	2-4
DOIs	https://doi.org/10.1007/s10509-009-9978-9
State	Published - Feb 2009

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/s10509-009-9978-9

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title = "Plasma magnetosphere formation around oscillating magnetized neutron stars",

abstract = "The notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission in the region of open field lines of plasma magnetosphere.",

author = "Ahmedov, {B. J.} and Morozova, {V. S.}",

note = "Funding Information: Acknowledgements This research is supported in part by the UzFFR (projects 5-08 and 29-08) and projects FA-F1-079, FA-F2-F061 and A13-226 of the UzAS, by the ICTP through the OEA-PRJ-29 and the Regular Associateship grants.",

year = "2009",

month = feb,

doi = "10.1007/s10509-009-9978-9",

language = "English (US)",

volume = "319",

pages = "115--117",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer Netherlands",

number = "2-4",

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T1 - Plasma magnetosphere formation around oscillating magnetized neutron stars

AU - Ahmedov, B. J.

AU - Morozova, V. S.

N1 - Funding Information: Acknowledgements This research is supported in part by the UzFFR (projects 5-08 and 29-08) and projects FA-F1-079, FA-F2-F061 and A13-226 of the UzAS, by the ICTP through the OEA-PRJ-29 and the Regular Associateship grants.

PY - 2009/2

Y1 - 2009/2

N2 - The notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission in the region of open field lines of plasma magnetosphere.

AB - The notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission in the region of open field lines of plasma magnetosphere.

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M3 - Article

AN - SCOPUS:59849121377

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SP - 115

EP - 117

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 2-4

ER -

Plasma magnetosphere formation around oscillating magnetized neutron stars

Abstract

All Science Journal Classification (ASJC) codes

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