Modelling pulsations of magnetic Ap stars

Hideyuki Saio

doi:10.1063/1.2993672

Modelling pulsations of magnetic Ap stars

Hideyuki Saio

Science

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Some chemically peculiar Ap stars with strong (a few kG) magnetic fields pulsate in high order p-modes modified by Lorentz forces. We review theoretical works for the pulsation of these stars, where including the magnetic effect makes the analysis considerably complicated.

Original language	English
Title of host publication	Exploring the Solar System and the Universe
Pages	337-343
Number of pages	7
DOIs	https://doi.org/10.1063/1.2993672
Publication status	Published - 2008 Oct 22
Event	Exploring the Solar System and the Universe - Bucharest, Romania Duration: 2008 Apr 8 → 2008 Apr 12

Publication series

Name	AIP Conference Proceedings
Volume	1043
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	Exploring the Solar System and the Universe
Country/Territory	Romania
City	Bucharest
Period	08/4/8 → 08/4/12

Keywords

Magnetic fields
Stellar oscillations

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.2993672

Cite this

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title = "Modelling pulsations of magnetic Ap stars",

abstract = "Some chemically peculiar Ap stars with strong (a few kG) magnetic fields pulsate in high order p-modes modified by Lorentz forces. We review theoretical works for the pulsation of these stars, where including the magnetic effect makes the analysis considerably complicated.",

keywords = "Magnetic fields, Stellar oscillations",

author = "Hideyuki Saio",

year = "2008",

month = oct,

day = "22",

doi = "10.1063/1.2993672",

language = "English",

isbn = "9780735405714",

series = "AIP Conference Proceedings",

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note = "Exploring the Solar System and the Universe ; Conference date: 08-04-2008 Through 12-04-2008",

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AB - Some chemically peculiar Ap stars with strong (a few kG) magnetic fields pulsate in high order p-modes modified by Lorentz forces. We review theoretical works for the pulsation of these stars, where including the magnetic effect makes the analysis considerably complicated.

KW - Magnetic fields

KW - Stellar oscillations

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U2 - 10.1063/1.2993672

DO - 10.1063/1.2993672

M3 - Conference contribution

AN - SCOPUS:54049113060

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T3 - AIP Conference Proceedings

SP - 337

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BT - Exploring the Solar System and the Universe

T2 - Exploring the Solar System and the Universe

Y2 - 8 April 2008 through 12 April 2008

ER -

Modelling pulsations of magnetic Ap stars

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

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