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Volumn 463, Issue 2, 2007, Pages 703-706

On the nature of the cool component of MWC 560

Author keywords

Infrared: stars; Stars: binaries: symbiotic; Stars: individual: MWC 560 (V694 Mon); Stars: late type; Stars: mass loss; Stars: oscillations

Indexed keywords

ASTROPHYSICS; INFRARED RADIATION; LIGHT EMISSION;

EID: 33847421393     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066538     Document Type: Article
Times cited : (17)

References (26)
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    • Fra̧ckowiak, S.M.1    Mikołajewski, M.2    Tomov, T.3
  • 16
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    • Podsiadlowski, P. 2007, in Evolution and chemistry of symbiotic stars, binary post-AGB and related objects, ed. J. Mikołajewska. & R. Szczerba, Baltic Astron., 16-1
    • Podsiadlowski, P. 2007, in Evolution and chemistry of symbiotic stars, binary post-AGB and related objects, ed. J. Mikołajewska. & R. Szczerba, Baltic Astron., 16-1
  • 20
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    • Schmid, H. M., Kaufer, A., Camenzind, M., et al. 2001, A&A, 377, 206 Szkody, P., Mateo, M., & Schmeer, P. 1990, IAU Circ., 4987
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  • 26
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    • Asymptotic Giant Branch Stars
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    • Winters, J. M., Le Bertre, T., & Keady, J. J. 1999, in Asymptotic Giant Branch Stars, ed. T. Le Bertre, A. Lebre, & C. Waelkens, IAU Symp., 191, 261
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    • Winters, J.M.1    Le Bertre, T.2    Keady, J.J.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.