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Volumn 358, Issue 3, 2000, Pages 1151-1156

The physical foundations of stellar magnetic field diagnosis from polarimetric observations of hydrogen lines

Author keywords

Line: formation; Polarization; Radiative transfer; Stars: atmospheres; Stars: magnetic fields

Indexed keywords


EID: 0009703148     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (18)

References (19)
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  • 3
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    • Ph.D. thesis, Univ. Paris XI
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    • (1999)
    • Brillant, S.1
  • 9
    • 0041876699 scopus 로고
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  • 12
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    • Mathys, G.1
  • 13
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    • Mathys G., 1983, A&A 125, 13
    • (1983) A&A , vol.125 , pp. 13
    • Mathys, G.1
  • 14
    • 0001879793 scopus 로고
    • Hydrogen line formation in dense plasmas in the presence of a magnetic field
    • Beckman J.E., Crivellari L. (eds.), Dordrecht: Reidel
    • Mathys G., 1985, Hydrogen line formation in dense plasmas in the presence of a magnetic field, in: Beckman J.E., Crivellari L. (eds.), Progress in Stellar Spectral Line Formation Theory, Dordrecht: Reidel, p. 381
    • (1985) Progress in Stellar Spectral Line Formation Theory , pp. 381
    • Mathys, G.1
  • 16
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    • Mathys G., 1991, A&AS 89, 121
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    • Mathys, G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.