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Volumn 88, Issue 1-3, 2004, Pages 17-20

Study of the magnetic field on four different luminosity hot stars: γPegasi, γOrionis, ωOrionis, and ζPersei

Author keywords

Hot stars; Magnetic field; Pulsation period; Radial velocity

Indexed keywords

RADIATIVE TRANSFER; STARS;

EID: 4444342919     PISSN: 00224073     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.jqsrt.2004.03.022     Document Type: Article
Times cited : (2)

References (8)
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  • 3
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    • Note on the period γ Pegasi
    • Sandberg HE. et al. Note on the period γ Pegasi. Publ Astron Soc Pacific 1960;72:508-9.
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    • Sandberg, H.E.1
  • 4
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    • Spectrographic observations of the β CMa variable star γ Pegasi
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    • Ducatel, D.1
  • 5
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    • Dynamics of the photosphere and shells in the β Cephei star γ Pegasi
    • Smith MA, McCall ML. Dynamics of the photosphere and shells in the β Cephei star γ Pegasi. Astrophys 1978;221:861-8.
    • (1978) Astrophys , vol.221 , pp. 861-868
    • Smith, M.A.1    McCall, M.L.2
  • 6
    • 0000059127 scopus 로고    scopus 로고
    • The magnetic field and wind confinement of β Cephei: New clues for interpreting the Be phenomenon?
    • Donati J-F. et al. The magnetic field and wind confinement of β Cephei: New clues for interpreting the Be phenomenon?. Mon Not Roy Astron Soc 2001;326:1265-78.
    • (2001) Mon Not Roy Astron Soc , vol.326 , pp. 1265-1278
    • Donati, J.-F.1
  • 7
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    • Discovery of a magnetic field in the Slowly Pulsating B star ζ Cassiopea
    • Neiner et al. Discovery of a magnetic field in the Slowly Pulsating B star ζ Cassiopea. Astron Astrophys 2003;406:1019-32.
    • (2003) Astron Astrophys , vol.406 , pp. 1019-1032
    • Neiner1
  • 8
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    • Stellar atmospheric velocity fields: The Beta Cephei variables γ Peg and β Cep
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    • De Jager1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.