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Volumn 48, Issue 2, 1996, Pages 305-315

Emission-line profiles from Be-star envelopes with m = 1 perturbation patterns

Author keywords

Line profiles; Stars: Be; Stars: circumstellar shells; Stars: emission lines; Stars: variable

Indexed keywords

EIGENVALUES AND EIGENFUNCTIONS; ELECTROMAGNETIC WAVE EMISSION;

EID: 0030534737     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/48.2.305     Document Type: Article
Times cited : (23)

References (33)
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    • Adam, J.1    Innes, D.E.2    Shaviv, G.3    Störzer, H.4    Wehrse, R.5
  • 9
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    • Hirata R., Hubert-Delplace A.-M. 1981, in Workshop on Pulsating B Stars, ed M. Auvergne, A. Baglin, D. Ducatel, J.-M. Le Contel, P.J. Morel, J.-P. Sareyan, J.-C. Valtier, C Sterken (Observatoire de Nice, Nice) p217
    • (1981) Workshop on Pulsating B Stars , pp. 217
    • Hirata, R.1    Hubert-Delplace, A.-M.2
  • 14
    • 33744701528 scopus 로고
    • Pulsation, Rotation, and Mass Loss of Early Type Stars, ed L.A. Balona, H.F. Henrichs, J.M. Le Contel (Kluwer Academic Publisher, Dordrecht)
    • Hummel W., Hanuschik R.W. 1994, in Pulsation, Rotation, and Mass Loss of Early Type Stars, IAU Symp. No. 162, ed L.A. Balona, H.F. Henrichs, J.M. Le Contel (Kluwer Academic Publisher, Dordrecht) p382
    • (1994) IAU Symp. No. 162 , vol.162 , pp. 382
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  • 15
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    • 0039915711 scopus 로고
    • ed F. Meyer, W. J. Duschl, J. Frank, E. Meyer-Hofmeister (Kluwer Academic Publishers, Dordrecht)
    • Kato S. 1989, in Theory of Accretion Disks, ed F. Meyer, W. J. Duschl, J. Frank, E. Meyer-Hofmeister (Kluwer Academic Publishers, Dordrecht) p173
    • (1989) Theory of Accretion Disks , pp. 173
    • Kato, S.1
  • 17
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    • Paper I
    • Okazaki A.T. 1991, PASJ 43, 75 (Paper I)
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    • Okazaki, A.T.1
  • 29
    • 33744675403 scopus 로고
    • ed M. Jaschek, H.-G. Groth (D. Reidel Publishing Company, Dordrecht)
    • Poeckert R. 1982, in Be stars, IAU Symp. No.98, ed M. Jaschek, H.-G. Groth (D. Reidel Publishing Company, Dordrecht), p453
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    • Poeckert, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.