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Volumn 325, Issue 2, 1997, Pages 551-558

Detection of planetary spectral features of extrasolar planets through their circumstellar dust - A Monte Carlo simulation

Author keywords

Infrared: solar system; Interplanetary medium; Methods: statistical; Planets and satellites: general; Radiative transfer; Stars: circumstellar matter; Stars: planetary systems

Indexed keywords


EID: 0142175499     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (2)

References (23)
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  • 3
    • 0006141755 scopus 로고
    • Modelling and understanding the dust around Beta Pictoris
    • Ferlet, R., Vidal-Madjar, A. (eds.), Editions Frontieres
    • Artymowicz, P., 1994, Modelling and understanding the dust around Beta Pictoris. In: Ferlet, R., Vidal-Madjar, A. (eds.), Circumstellar dust disks and planet formation. Editions Frontieres, p. 47
    • (1994) Circumstellar Dust Disks and Planet Formation , pp. 47
    • Artymowicz, P.1
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    • Polarization by Circumstellar dust - Modelling and Interpretation of Polarization Maps
    • 1995
    • Fischer, O., 1995, Polarization by Circumstellar dust - Modelling and Interpretation of Polarization Maps. In: Reviews in Modern Astronomy, Vol. 7, 1995, p. 103
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    • Fischer, O.1
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    • (1990) Physics of the Inner Heliosphere , vol.1 , pp. 236
    • Leinert, Ch.1    Grün, E.2
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    • Sandford, S. A., 1988. In: Bailey, M. E. & Williams, D. A. (eds.), Dust in the Universe. Cambridge University Press, Cambridge, p. 193
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    • Sandford, S.A.1
  • 19
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    • Overview of detection methods
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    • Schneider, J.1
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    • (1996) Nature , vol.382 , pp. 23
    • Walker, G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.